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<ri:Resource created="2023-11-16T10:32:41Z" 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>Census of circumgalactic MgII at redshift z=&lt;0.5</title><shortName>J/MNRAS/502/4743</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/502/4743</identifier><altIdentifier>doi:10.26093/cds/vizier.75024743</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Huang Y.-H.</name></creator><creator><name>Chen H.-W.</name></creator><creator><name>Shectman S.A.</name></creator><creator><name>Johnson S.D.</name></creator><creator><name>Zahedy F.S.,Helsby J.E.</name></creator><creator><name>Gauthier J.-R.</name></creator><creator><name>Thompson I.B.</name></creator><date role="Updated">2024-08-21T20:17:13Z</date><date role="Created">2023-11-16T10:32:41Z</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>quasars</subject><subject>redshifted</subject><subject>line-intensities</subject><subject>spectroscopy</subject><subject>ultraviolet-astronomy</subject><subject>visible-astronomy</subject><description>This paper presents a survey of MgII absorbing gas in the vicinity of 380 random galaxies, using 156 background quasi-stellar objects (QSOs) as absorption-line probes. The sample comprises 211 isolated (73 quiescent and 138 star-forming galaxies) and 43 non-isolated galaxies with sensitive constraints for both MgII absorption and H{alpha} emission. The projected distances span a range from d=9 to 497kpc, redshifts of the galaxies range from z=0.10 to 0.48, and rest-frame absolute B-band magnitudes range from M_B_=-16.7 to -22.8. Our analysis shows that the rest-frame equivalent width of MgII, W_r_(2796), depends on halo radius (R_h_), B-band luminosity(L_B_), and stellar mass (M_star_) of the host galaxies, and declines steeply with increasing d for isolated, star-forming galaxies. At the same time, W_r_(2796) exhibits no clear trend for either isolated, quiescent galaxies or non-isolated galaxies. In addition, the covering fraction of MgII absorbing gas &lt;{kappa}&gt; is high with &lt;{kappa}&gt;&gt;=60 per cent at &lt;40kpc for isolated galaxies and declines rapidly to &lt;{kappa}&gt;~0 at d&gt;=100 kpc. Within the gaseous radius, the incidence of MgII gas depends sensitively on both M_star_ and the specific star formation rate inferred from H{alpha}. Different from what is known for massive quiescent haloes, the observed velocity dispersion of MgII absorbing gas around star-forming galaxies is consistent with expectations from virial motion, which constrains individual clump mass to m_cl_&gt;~10^5^M_{sun}_ and cool gas accretion rate of ~0.7-2M_{sun}_/yr. Finally, we find no strong azimuthal dependence of MgII absorption for either star-forming or quiescent galaxies. Our results demonstrate that multiple parameters affect the properties of gaseous haloes around galaxies and highlight the need of a homogeneous, absorption-blind sample for establishing a holistic description of chemically enriched gas in the circumgalactic space.</description><source format="bibcode">2021MNRAS.502.4743H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/502/4743</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/II/294">II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 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27229 27251 27254 27310 27320 27332 27349 27396 27398 27467 27497 27512 27526 27542 27548 27587 27709 27722 27739 27789 27791 27818 27862 27932 30040 30042 30046 31311 31331 31393 31434 31454 31476 31622 36723 36784 36789 36792 36802 49015 49085 49122</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/502/4743?format=ascii</footprint><waveband>UV</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/502/4743/table1</name><description>Summary of Faint Galaxy Spectroscopy</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="24*">char</dataType><flag>nullable</flag></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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