<?xml-stylesheet href='/static/xsl/oai.xsl' type='text/xsl'?>
<ri:Resource created="2020-12-17T12:36:54Z" 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>Half-mass radii for ~7000 galaxies at 1.0&lt;=z&lt;=2.5</title><shortName>J/ApJ/877/103</shortName><identifier>ivo://CDS.VizieR/J/ApJ/877/103</identifier><altIdentifier>doi:10.26093/cds/vizier.18770103</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Suess K.A.</name></creator><creator><name>Kriek M.</name></creator><creator><name>Price S.H.</name></creator><creator><name>Barro G.</name></creator><date role="Updated">2021-03-29T12:23:36Z</date><date role="Created">2020-12-17T12:36:54Z</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>galaxy-classification-systems</subject><subject>redshifted</subject><description>Radial mass-to-light ratio gradients cause the half-mass and half-light radii of galaxies to differ, potentially biasing studies that use half-light radii. Here we present the largest catalog to date of galaxy half-mass radii at z&gt;1: 7006 galaxies in the CANDELS fields at 1.0&lt;=z&lt;=2.5. The sample includes both star-forming and quiescent galaxies with stellar masses 9.0&lt;=log(M_*_/M_{sun}_)&lt;=11.5. We test three methods for calculating half-mass radii from multiband PSF-matched Hubble Space Telescope (HST) imaging: two based on spatially resolved spectral energy distribution modeling, and one that uses a rest-frame color profile. All three methods agree, with scatter &lt;~0.3dex. In agreement with previous studies, most galaxies in our sample have negative color gradients (the centers are redder than the outskirts, and r_e,mass_&lt;r_e,light_). We find that color gradient strength has significant trends with increasing stellar mass, half-light radius, U-V color, and stellar mass surface density. These trends have not been seen before at z&gt;1. Furthermore, color gradients of star-forming and quiescent galaxies show a similar redshift evolution: they are flat at z&gt;~2, then steeply decrease as redshift decreases. This affects the galaxy mass-size relation. The normalizations of the star-forming and quiescent r_mass_-M_*_ relations are 10%-40% smaller than the corresponding r_light_-M_*_ relations; the slopes are ~0.1-0.3dex shallower. Finally, the half-mass radii of star-forming and quiescent galaxies at M_*_=10^10.5^M_{sun}_ only grow by ~1% and ~8% between z~2.25 and z~1.25. This is significantly less than the ~37% and ~47% size increases found when using the half-light radius.</description><source format="bibcode">2019ApJ...877..103S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/877/103</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/ApJ/655/51">J/ApJ/655/51 : HDFS IRAC observations of 2&lt;z&lt;3.5 galaxies (Wuyts+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/739/L44">J/ApJ/739/L44 : Structural data for gal. between 0.2&lt;z&lt;2.7 (Damjanov+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/749/121">J/ApJ/749/121 : Surface brightness profiles if z=2 galaxies (Szomoru+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/203/24">J/ApJS/203/24 : Structural parameters of gal. in CANDELS (van der Wel+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/206/10">J/ApJS/206/10 : CANDELS multiwavelength catalog (Galametz+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/73">J/ApJ/763/73 : Surface density profiles of GOODS-South gal. (Szomoru+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/771/85">J/ApJ/771/85 : Dynamical masses of z~2 quiescent gal. (van de Sande+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/214/24">J/ApJS/214/24 : 3D-HST+CANDELS catalog (Skelton+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/225/27">J/ApJS/225/27 : 3D-HST Survey: grism spectra master catalog (Momcheva+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/830/51">J/ApJ/830/51 : FourStar galaxy evolution survey (ZFOURGE) (Straatman+, 2016)</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/877/103</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/877/103</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/877/103</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/877/103</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/877/103</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/877/103</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/877/103/table1 (Half-mass radii for 7006 galaxies)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/877/103/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/877/103/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/877/103/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>34.33022306</ra><dec>-5.21306611</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/17679 17690 27258 35935</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/877/103?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/877/103/table1</name><description>Half-mass radii for 7006 galaxies</description><column><name>isQui</name><description>Galaxy classified as quiescent (7)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">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>ID</name><description>[161/50461] 3D-HST catalog (v4.0) identifier (&lt;[SWM2014] {Field} NNNNN&gt; in Simbad)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Field</name><description>Field identifier (COSMOS, GOODS-S or UDS)</description><ucd>meta.id;obs.field</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>RAJ2000</name><description>[34.22/150.21] Right Ascension (J2000) (1)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[-27.9/2.4] Declination (J2000) (1)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>z</name><description>[1/2.5] Photometric redshift (2)</description><ucd>src.redshift.phot</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logM*</name><description>[9/11.8] log stellar mass (3)</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>re</name><description>[0.14/208.4]? Effective half light radius (4)</description><unit>kpc</unit><ucd>phys</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_re</name><description>[0/71.2]? Uncertainty in re</description><unit>kpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n</name><description>[0.2/8] Sersic index (5)</description><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_n</name><description>[0/4.7] Uncertainty in n (5)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>rem1</name><description>[0.15/79.3]? Method 1 effective half mass radius (6)</description><unit>kpc</unit><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_rem1</name><description>[0.14/66.4]? Lower 16% percentile uncertainty in rem1</description><unit>kpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_rem1</name><description>[0.18/99.5]? Upper 84% percentile uncertainty in rem1</description><unit>kpc</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>rem2</name><description>[0.25/203.2]? Method 2 effective half mass radius (6)</description><unit>kpc</unit><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_rem2</name><description>[0.25/203]? Lower 16% percentile uncertainty in rem2</description><unit>kpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_rem2</name><description>[0.28/203.4]? Upper 84% percentile uncertainty in rem2</description><unit>kpc</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>rem3</name><description>[0.14/58.3]? Method 3 effective half mass radius (6)</description><unit>kpc</unit><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_rem3</name><description>[0.14/50.9]? Lower 16% percentile uncertainty in rem3</description><unit>kpc</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>E_rem3</name><description>[0.15/100]? Upper 84% percentile uncertainty in rem3</description><unit>kpc</unit><ucd>stat.error;stat.max</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>ZFOURGE</name><description>Display data from ZFOURGE (Straatman+, 2016, J/ApJ/830/51) within 0.5"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>vdW12</name><description>Display data from van der Wel+, 2012, J/ApJS/203/24 within 0.5"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>