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<ri:Resource created="2021-02-10T07:43:01Z" 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>HST phot. &amp; GMOS spectra of Lynx E &amp; W clusters</title><shortName>J/ApJ/881/42</shortName><identifier>ivo://CDS.VizieR/J/ApJ/881/42</identifier><altIdentifier>doi:10.26093/cds/vizier.18810042</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Jorgensen I.</name></creator><creator><name>Hunter L.C.</name></creator><creator><name>O'Neill C.R.</name></creator><creator><name>Chiboucas K.</name></creator><creator><name>Cole R.K.</name></creator><creator><name>Toft S.,Schiavon R.P.</name></creator><date role="Updated">2022-05-05T13:42:06Z</date><date role="Created">2021-02-10T07:43:01Z</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>hst-photometry</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>galaxy-clusters</subject><subject>redshifted</subject><subject>galaxies</subject><subject>line-intensities</subject><subject>galaxy-kinematics</subject><subject>x-ray-sources</subject><description>Few detailed investigations of stellar populations in passive galaxies beyond z~1 are based on deep spectroscopic observations, due to the difficulty in obtaining such data. We present a study of stellar populations, structure, and mass-to-light ratios (M/L) of a large sample of bulge-dominated galaxies in the two z=1.27 clusters Lynx E and Lynx W, based on deep ground-based optical spectroscopy combined with imaging from the Hubble Space Telescope. We find that Lynx E has a well-defined core of red passive galaxies, while Lynx W lacks such a core. If all the sample galaxies evolve similarly in size from z=1.27 to the present, the data would allow only 0.1dex size growth at a fixed dynamical mass. However, to link the Lynx central galaxies to brightest cluster galaxies similar to those of low-redshift clusters, the Lynx galaxies would have to grow by at least a factor 5, possibly through major merging. The M/L ratios and the Balmer absorption lines of the Lynx galaxies are consistent with passive evolution of the stellar populations from z=1.27 to the present and support ages of 1-3Gyr. The galaxies in the outskirts of the clusters contain younger stellar populations than found in the cluster cores. However, when evolved passively to z~0 both populations are consistent with the observed populations in the Coma cluster galaxies. The bulge-dominated emission line galaxies in the clusters are dominated by stellar populations with subsolar metallicities. Thus, additional enrichment of these is required to produce Coma-like stellar populations by z~0.</description><source format="bibcode">2019ApJ...881...42J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/881/42</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/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/71/549">J/ApJS/71/549 : Case low-dispersion Survey X. 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Total magnitude from r^1/4^ fit in F850LP (1)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logRe-dev</name><description>[-1.13/0.54]? Log of the effective radius from r^1/4^ fit in F850LP</description><unit>log(arcsec)</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>z'ser</name><description>[21/26]? Total magnitude from Sersic fit in F850LP (1)</description><unit>mag</unit><ucd>phot.mag;em.opt.I</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>logRe-ser</name><description>[-1.12/0.021]? Log of the effective radius from Sersic fit in F850LP</description><unit>log(arcsec)</unit><ucd>phys.angSize</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>nser</name><description>[0.3/7]? 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Cluster</name><description>Cluster name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>z</name><description>[1.26/1.271] Cluster redshift, adopting BCGs as cluster centers (1)</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>sigma</name><description>[568/693] Cluster velocity dispersion, adopting BCGs as cluster centers</description><unit>km/s</unit><ucd>phys.veloc.dispersion</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_sigma</name><description>[87/90] Negative uncertainty on sigma</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>E_sigma</name><description>[67/68] Positive uncertainty on sigma</description><unit>km/s</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Nmm</name><description>[15/24] Number of member galaxies for which spectroscopy is available, adopting BCGs as cluster centers</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>zX</name><description>[1.26/1.271] Cluster redshift, adopting X-ray centers (2)</description><ucd>src.redshift;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>sigmaX</name><description>[580/706] velocity dispersion, adopting X-ray centers (2)</description><unit>km/s</unit><ucd>phys.veloc.dispersion</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_sigmaX</name><description>[77/79] Negative uncertainty on sigmaX</description><unit>km/s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>E_sigmaX</name><description>[65/83] Positive uncertainty on sigmaX</description><unit>km/s</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>NmmX</name><description>[16/23] Number of member galaxies, when adopting X-ray centers (2)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>L500</name><description>[0.63/3.73] X-ray luminosity in the 0.1-2.4keV band within the radius R500, in 10^44^erg/s (2)</description><unit>1e+37W</unit><ucd>phys.luminosity;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>M500</name><description>[0.55/1.65] Cluster mass derived from X-ray data within the radius R500 (2)</description><unit>1e+14solMass</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>R500</name><description>[0.35/0.52] Radius within which the mean overdensity of the cluster is 500 times the critical density at the cluster redshift</description><unit>Mpc</unit><ucd>phys.size.radius</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table><table><name>J/ApJ/881/42/table10</name><description>Spectroscopic parameters</description><column><name>CN3883</name><description>[0.06/0.4]? 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Uncertainty in CN3883 (5)</description><unit>mag</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>CaHK</name><description>[5.2/24.6]? The CaHK line index (4)</description><unit>0.1nm</unit><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_CaHK</name><description>[0.2/1.4]? Uncertainty in CaHK (5)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>D4000</name><description>[1.2/2.2]? The D4000 line index (4)</description><ucd>spect.index;spect.line</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_D4000</name><description>[0.002/0.014]? Uncertainty in D4000 (5)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>HzetaA</name><description>[1.5/6.5]? The H_{zeta}A_ line index (4)</description><unit>0.1nm</unit><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_HzetaA</name><description>[0.08/0.5]? Uncertainty in HzetaA (5)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>EWOII</name><description>[2.9/163]? Equivalent width of the [OII] emission if present</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_EWOII</name><description>[0.2/78]? Uncertainty on EWOII</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>