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<ri:Resource created="2020-06-13T09:41:33Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>CLASH galaxies photometric redshifts in 25 ClG</title><shortName>J/MNRAS/470/95</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/470/95</identifier><altIdentifier>doi:10.26093/cds/vizier.74700095</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Molino A.</name></creator><creator><name>Benitez N.</name></creator><creator><name>Ascaso B.</name></creator><creator><name>Coe D.</name></creator><creator><name>Postman M.</name></creator><creator><name>Jouvel S.</name></creator><creator><name>Host O.,Lahav O.</name></creator><creator><name>Seitz S.</name></creator><creator><name>Medezinski E.</name></creator><creator><name>Rosati P.</name></creator><creator><name>Schoenell W.</name></creator><creator><name>Koekemoer A.,Jimenez-teja Y.</name></creator><creator><name>Broadhurst T.</name></creator><creator><name>Melchior P.</name></creator><creator><name>Balestra I.</name></creator><creator><name>Bartelmann M.,Bouwens R.</name></creator><creator><name>Bradley L.</name></creator><creator><name>Czakon N.</name></creator><creator><name>Donahue M.</name></creator><creator><name>Ford H.</name></creator><creator><name>Graur O.,Graves G.</name></creator><creator><name>Grillo C.</name></creator><creator><name>Infante L.</name></creator><creator><name>Jha S.W.</name></creator><creator><name>Kelson D.</name></creator><creator><name>Lazkoz R.</name></creator><creator><name>Lemze D.,Maoz D.</name></creator><creator><name>Mercurio A.</name></creator><creator><name>Meneghetti M.</name></creator><creator><name>Merten J.</name></creator><creator><name>Moustakas L.</name></creator><creator><name>Nonino M.,Orgaz S.</name></creator><creator><name>Riess A.</name></creator><creator><name>Rodney S.</name></creator><creator><name>Sayers J.</name></creator><creator><name>Umetsu K.</name></creator><creator><name>Zheng W.</name></creator><creator><name>Zitrin A.</name></creator><date role="Updated">2024-08-17T20:20:05Z</date><date role="Created">2020-06-13T09:41:33Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>galaxy-clusters</subject><subject>galaxies</subject><subject>photometry</subject><subject>redshifted</subject><description>We present accurate photometric redshifts for galaxies observed by the Cluster Lensing And Supernova survey with Hubble (CLASH). CLASH observed 25 massive galaxy cluster cores with the Hubble Space Telescope in 16 filters spanning 0.2-1.7{mu}m. Photometry in such crowded fields is challenging. Compared to our previously released catalogues, we make several improvements to the photometry, including smaller apertures, intracluster light subtraction, point spread function matching and empirically measured uncertainties. We further improve the Bayesian photometric redshift estimates by adding a redder elliptical template and by inflating the photometric uncertainties of the brightest galaxies. The resulting photometric redshift accuracies are dz/(1+z)~0.8, 1.0 and 2.0 per cent for galaxies with I-band F814W AB magnitudes &lt;18, 20 and 23, respectively. These results are consistent with our expectations. They improve on our previously reported accuracies by a factor of 4 at the bright end and a factor of 2 at the faint end. Our new catalogue includes 1257 spectroscopic redshifts, including 382 confirmed cluster members. We also provide stellar mass estimates. Finally, we include lensing magnification estimates of background galaxies based on our public lens models. Our new catalogue of all 25 CLASH clusters is available via Mikulski Archive for Space Telescopes. The analysis techniques developed here will be useful in other surveys of crowded fields, including the Frontier Fields and surveys carried out with Javalambre-Physics of the Accelerated Universe Astrophysical Survey and James Webb Space Telescope.</description><source format="bibcode">2017MNRAS.470...95M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/470/95</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource>https://archive.stsci.edu/prepds/clash : CLASH home 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F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? 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F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/table1</name><description>The CLASH galaxy cluster sample</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="16*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Cluster name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="17*">char</dataType></column><column><name>z</name><description>Mean spectroscopic redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Ngal</name><description>Number of galaxies in the associated catalog</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Cluster</name><description>Cluster short name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column></table><table><name>J/MNRAS/470/95/a383</name><description>Abell 383 photometric redshift catalogue</description><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/a209</name><description>Abell 209 photometric redshift catalogue</description><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/a1423</name><description>Abell 1423 photometric redshift catalogue</description><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/a2261</name><description>Abell 2261 photometric redshift catalogue</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/rxj2129</name><description>RX J2129+0005 photometric redshift catalogue</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/a611</name><description>Abell 611 photometric redshift catalogue</description><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/ms2137</name><description>MS2137-2353 photometric redshift catalogue</description><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/rxj1532</name><description>RX J1532.8+3021 photometric redshift catalogue</description><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/rxj2248</name><description>RX J2248-4431 photometric redshift catalogue</description><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/macs1931</name><description>MACS J1931-26 photometric redshift catalogue</description><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/macs1115</name><description>MACS J1115+0129 photometric redshift catalogue</description><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/macs1720</name><description>MACS J1720+3536 photometric redshift catalogue</description><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/macs0429</name><description>MACS J0429-02 photometric redshift catalogue</description><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/macs0416</name><description>MACS J0416-24 photometric redshift catalogue</description><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/macs1206</name><description>MACS J1206-08 photometric redshift catalogue</description><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/macs0329</name><description>MACS J0329-02 photometric redshift catalogue</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/macs1311</name><description>MACS J1311-03 photometric redshift catalogue</description><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/macs1423</name><description>MACS J1423.8+2404 photometric redshift catalogue</description><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/macs1149</name><description>MACS J1149+22 photometric redshift catalogue</description><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/macs0717</name><description>MACS J0717+37 photometric redshift catalogue</description><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/macs2129</name><description>MACS J2129+0005 photometric redshift catalogue</description><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/macs0647</name><description>MACS J0647+70 photometric redshift catalogue</description><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/macs0744</name><description>MACS J0744+39 photometric redshift catalogue</description><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table><table><name>J/MNRAS/470/95/clj1226</name><description>CL J1226+3332 photometric redshift catalogue</description><column><name>rp</name><description>Petrosian radii</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rk</name><description>Kron-apertures in units of A or B</description><unit>pix</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>CLASHID</name><description>Object ID Number [clash_*cluster*_nir_*SExtID*]</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>Cluster</name><description>Cluster short Name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="8*">char</dataType></column><column><name>RAJ2000</name><description>Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Xpos</name><description>X-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.x</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Ypos</name><description>Y-pixel coordinate</description><unit>pix</unit><ucd>pos.cartesian.y</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Area</name><description>Isophotal aperture area (pixels)</description><unit>pix</unit><ucd>phys.area;instr</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>FWHM</name><description>Full width at half maximum for detection image</description><unit>arcsec</unit><ucd>spect.line.width</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>s2n</name><description>Signal to Noise (SExt_FLUX_AUTO/SExt_FLUXERR_AUTO)</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>photFlag</name><description>SExtractor Photometric Flag</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfobs</name><description>Number Filters Observed (out of 24)</description><ucd>meta.number;phys.atmol.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>nfdet</name><description>Number Filters Detected (out of 24)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>PS</name><description>[0/1] Pointsource flag (0: extended / 1: point-like)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>theta</name><description>Position Angle (CCW/x)</description><ucd>pos.posAng</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>a</name><description>Profile RMS along major axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>b</name><description>Profile RMS along minor axis</description><unit>pix</unit><ucd>stat.stdev</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Backg</name><description>Background-signal subtracted from Detection</description><ucd>instr.background</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rf</name><description>Fraction-of-light radii</description><unit>pix</unit><ucd>src.morph.scLength</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>RABdeg</name><description>BCG position in Right Ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra</ucd></column><column><name>DEBdeg</name><description>BCG position in Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec</ucd></column><column><name>PDistBCG</name><description>Projected Physical Distance to BCG</description><unit>Mpc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F225WPZ</name><description>? F225W/WFC3 restricted magnitude (AB); best for photo-z (F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WPZ</name><description>F225W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F225W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F225WM</name><description>? F225W/WFC3 moderated magnitude (AB); best for stellar mass (F225W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F225WM</name><description>F225W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F225W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WPZ</name><description>? F275W/WFC3 restricted magnitude (AB); best for photo-z (F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WPZ</name><description>F275W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F275W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F275WM</name><description>? F275W/WFC3 moderated magnitude (AB); best for stellar mass (F275W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.200-300nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F275WM</name><description>F275W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F275W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WPZ</name><description>? F336W/WFC3 restricted magnitude (AB); best for photo-z (F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WPZ</name><description>F336W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F336W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F336WM</name><description>? F336W/WFC3 moderated magnitude (AB); best for stellar mass (F336W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F336WM</name><description>F336W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F336W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WPZ</name><description>? F390W/WFC3 restricted magnitude (AB); best for photo-z (F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WPZ</name><description>F390W/WFC3 restricted magnitude uncertainty (AB); best for photo-z (e_F390W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F390WM</name><description>? F390W/WFC3 moderated magnitude (AB); best for stellar mass (F390W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.U</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F390WM</name><description>F390W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F390W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WPZ</name><description>? F435W/ACS restricted magnitude (AB) best for photo-z (F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WPZ</name><description>F435W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F435W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F435WM</name><description>? F435W/ACS moderated magnitude (AB) best for stellar mass (F435W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F435WM</name><description>F435W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F435W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WPZ</name><description>? F475W/ACS restricted magnitude (AB) best for photo-z (F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WPZ</name><description>F475W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F475W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F475WM</name><description>? F475W/ACS moderated magnitude (AB) best for stellar mass (F475W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F475WM</name><description>F475W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F475W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WPZ</name><description>? F606W/ACS restricted magnitude (AB) best for photo-z (F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WPZ</name><description>F606W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F606W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F606WM</name><description>? F606W/ACS moderated magnitude (AB) best for stellar mass (F606W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F606WM</name><description>F606W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F606W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WPZ</name><description>? F625W/ACS restricted magnitude (AB) best for photo-z (F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WPZ</name><description>F625W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F625W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F625WM</name><description>? F625W/ACS moderated magnitude (AB) best for stellar mass (F625W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F625WM</name><description>F625W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F625W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WPZ</name><description>? F775W/ACS restricted magnitude (AB) best for photo-z (F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WPZ</name><description>F775W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F775W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F775WM</name><description>? F775W/ACS moderated magnitude (AB) best for stellar mass (F775W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F775WM</name><description>F775W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F775W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WPZ</name><description>? F814W/ACS restricted magnitude (AB) best for photo-z (F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WPZ</name><description>F814W/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F814W_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F814WM</name><description>? F814W/ACS moderated magnitude (AB) best for stellar mass (F814W_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F814WM</name><description>F814W/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F814W_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPPZ</name><description>? F850LP/ACS restricted magnitude (AB) best for photo-z (F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPPZ</name><description>F850LP/ACS restricted magnitude uncertainty (AB) best for photo-z (e_F850LP_ACS_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F850LPM</name><description>? F850LP/ACS moderated magnitude (AB) best for stellar mass (F850LP_ACS_MASS)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F850LPM</name><description>F850LP/ACS moderated magnitude uncertainty (AB) best for stellar mass (e_F850LP_ACS_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WPZ</name><description>? F105W/WFC3 restricted magnitude (AB) best for photo-z (F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WPZ</name><description>F105W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F105W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F105WM</name><description>? F105W/WFC3 moderated magnitude (AB) best for stellar mass (F105W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F105WM</name><description>F105W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F105W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WPZ</name><description>? F110W/WFC3 restricted magnitude (AB) best for photo-z (F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WPZ</name><description>F110W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F110W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F110WM</name><description>? F110W/WFC3 moderated magnitude (AB) best for stellar mass (F110W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F110WM</name><description>F110W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F110W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F125WPZ</name><description>? F125W/WFC3 restricted magnitude (AB) best for photo-z (F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WPZ</name><description>F125W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F125W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F125WM</name><description>? F125W/WFC3 moderated magnitude (AB) best for stellar mass (F125W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.J</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F125WM</name><description>F125W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F125W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WPZ</name><description>? F140W/WFC3 restricted magnitude (AB) best for photo-z (F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WPZ</name><description>F140W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F140W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F140WM</name><description>? F140W/WFC3 moderated magnitude (AB) best for stellar mass (F140W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.IR.H</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F140WM</name><description>F140W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F140W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F160WPZ</name><description>? F160W/WFC3 restricted magnitude (AB) best for photo-z (F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WPZ</name><description>F160W/WFC3 restricted magnitude uncertainty (AB) best for photo-z (e_F160W_WFC3_PHOTOZ)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>F160WM</name><description>? F160W/WFC3 moderated magnitude (AB) best for stellar mass (F160W_WFC3_MASS)</description><unit>mag</unit><ucd>phot.mag;em.UV.100-200nm</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_F160WM</name><description>F160W/WFC3 moderated magnitude uncertainty (AB) best for stellar mass (e_F160W_WFC3_MASS)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zCluster</name><description>Cluster Redshift</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zb1</name><description>[0/10] BPZ most likely redshift for the First Peak</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_zb1</name><description>Lower limit (95p confidence) for the First Peak</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>E_zb1</name><description>Upper limit (95p confidence) for the First Peak</description><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tb1</name><description>BPZ most likely spectral type for the First Peak</description><ucd>src.spType</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Odds1</name><description>P(z) contained within zb+/-2*0.03*(1+z) for the First Peak</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Chi2</name><description>Poorness of BPZ fit: observed vs. model fluxes</description><ucd>stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>BMAG</name><description>Absolute magnitude (AB) (B_JOHNSON) for the First Peak</description><unit>mag</unit><ucd>phys.magAbs;em.opt.B</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>? Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>F814W</name><description>? Lensing-corrected F814WM magnitude (F814W_ACS_MASS_LensCor)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>BMAGLC</name><description>? Lensing-corrected Absolute Magnitude (AB) (B_JOHNSON) (MB_LensCor)</description><unit>mag</unit><ucd>phys.magAbs</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logM*LC</name><description>? Lensing-corrected Stellar Mass for the First Peak (log10(M_sun))</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zsp</name><description>? Spectroscopic Redshift [-99 if unknown]</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_zsp</name><description>Reference for the Spectroscopic Redshift</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="13*">char</dataType></column><column><name>q_zsp</name><description>[0/2]? Quality of the Spectroscopic Redshift [0:secure, 1:likely, 2:unsure] (1)</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>