<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2001-05-11T11:51:20Z" 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>HDF photometric redshifts catalog</title><shortName>J/ApJ/513/34</shortName><identifier>ivo://CDS.VizieR/J/ApJ/513/34</identifier><altIdentifier>doi:10.26093/cds/vizier.15130034</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fernandez-Soto A.</name></creator><creator><name>Lanzetta K.M.</name></creator><creator><name>Yahil A.</name></creator><date role="Updated">2001-05-11T11:51:29Z</date><date role="Created">2001-05-11T11:51:20Z</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>galaxies</subject><subject>photometry</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>redshifted</subject><description>Using the newly available infrared images of the Hubble Deep Field in the J, H, and K bands and an optimal photometric method, we have refined a technique to estimate the redshifts of 1067 galaxies. A detailed comparison of our results with the spectroscopic redshifts in those cases where the latter are available shows that this technique gives very good results for bright enough objects [AB(814nm)&lt;26.0]. From a study of the distribution of residuals [{Delta}z_rms_/(1+z)~0.1 at all redshifts], we conclude that the observed errors are mainly due to cosmic variance. This very important result allows for the assessment of errors in quantities to be directly or indirectly measured from the catalog. We present some of the statistical properties of the ensemble of galaxies in the catalog, and we finish by presenting a list of bright high-redshift (z~5) candidates extracted from our catalog together with recent spectroscopic redshift determinations confirming that two of them are at z=5.34 and z=5.60.</description><source format="bibcode">1999ApJ...513...34F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/513/34</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 ivo-id="ivo://CDS.VizieR/J/AJ/112/1335">J/AJ/112/1335 : Hubble Deep Field observations (Williams+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/129/583">J/A+AS/129/583 : Hubble Deep Field surface photometry (Fasano+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/112/359">J/AJ/112/359 : Galaxies of the Hubble Deep Field (van den Bergh+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/116/2081">J/AJ/116/2081 : Hubble Deep Field catalog of color-based redshift (Wang+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/117/17">J/AJ/117/17 : Hubble Deep Field near-IR obs. (Thompson+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/453/48">J/ApJ/453/48 : VI photometry of HST faint field galaxies (Driver+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/471/L5">J/ApJ/471/L5 : Redshift clustering in the Hubble Deep Field (Cohen+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/507/585">J/ApJ/507/585 : Hubble Deep Field galaxy morphology (Marleau+, 1998)</relatedResource><relatedResource>Table 3: Stars in the Hubble Deep Field</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/513/34</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/513/34</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/513/34</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/513/34</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/513/34</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/513/34</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/513/34/table4 (*Coordinates, best AB(814nm) magnitudes, redshifts, and best-fit spectral types for every galaxy in the catalog)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/513/34/table4?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/513/34/table4?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/513/34/table4?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>189.2394875</ra><dec>62.20293333</dec><sr>0.005555555555555556</sr></testQuery></capability><facility>HST</facility><coverage><spatial>6/11252</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/513/34?format=ascii</footprint><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/513/34/table4</name><description>*Coordinates, best AB(814nm) magnitudes, redshifts, and best-fit spectral types for every galaxy in the catalog</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>[FLY99]</name><description>Identification number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>primary</flag></column><column><name>Xpos</name><description>X position on the mosaic image</description><unit>pix</unit><ucd>pos.cartesian.x;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Ypos</name><description>Y position on the mosaic image</description><unit>pix</unit><ucd>pos.cartesian.y;instr.det</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>[WBD96]</name><description>Williams et al., 1996 (Cat. &lt;J/AJ/112/1335&gt;) identification</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="14*">char</dataType></column><column><name>ABmag</name><description>AB(814nm) best magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zsp</name><description>? Spectoscopic redshift (if available)</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>zph</name><description>Photometric redshift (1)</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Type</name><description>[1/4] Best fit type (1=Ell, 2=Sbc, 3=Scd, 4=Irr)</description><ucd>meta.id;stat.fit</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/ApJ/513/34/table5</name><description>UBVIJHK fluxes and errors</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>[FLY99]</name><description>Identification number (1)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SU300</name><description>U band flux (2)</description><unit>nJy</unit><ucd>phot.flux;em.UV</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SU300</name><description>rms uncertainty on SU</description><unit>nJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SB450</name><description>B band flux (2)</description><unit>nJy</unit><ucd>phot.flux.density;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SB450</name><description>rms uncertainty on SB</description><unit>nJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SV606</name><description>V band flux (2)</description><unit>nJy</unit><ucd>phot.flux.density;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SV606</name><description>rms uncertainty on SV</description><unit>nJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SI814</name><description>I band flux (2)</description><unit>nJy</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_SI814</name><description>rms uncertainty on SI</description><unit>nJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>SJ</name><description>J band flux (2)</description><unit>nJy</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_SJ</name><description>? rms uncertainty on SJ</description><unit>nJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>SH</name><description>H band flux (2)</description><unit>nJy</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_SH</name><description>? rms uncertainty on SH</description><unit>nJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>SK</name><description>K band flux (2)</description><unit>nJy</unit><ucd>phot.flux.density;em.IR</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_SK</name><description>? rms uncertainty on SK</description><unit>nJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>