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<ri:Resource created="2018-03-08T15:33:02Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>Investigating Tully-Fisher relation with KMOS^3D^</title><shortName>J/ApJ/842/121</shortName><identifier>ivo://CDS.VizieR/J/ApJ/842/121</identifier><altIdentifier>doi:10.26093/cds/vizier.18420121</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ubler H.</name></creator><creator><name>Forster Schreiber N.M.</name></creator><creator><name>Genzel R.</name></creator><creator><name>Wisnioski E.</name></creator><creator><name>Wuyts S.,Lang P.</name></creator><creator><name>Naab T.</name></creator><creator><name>Burkert A.</name></creator><creator><name>van Dokkum P.G.</name></creator><creator><name>Tacconi L.J.</name></creator><creator><name>Wilman D.J.,Fossati M.</name></creator><creator><name>Mendel J.T.</name></creator><creator><name>Beifiori A.</name></creator><creator><name>Belli S.</name></creator><creator><name>Bender R.</name></creator><creator><name>Brammer G.B.,Chan J.</name></creator><creator><name>Davies R.</name></creator><creator><name>Fabricius M.</name></creator><creator><name>Galametz A.</name></creator><creator><name>Lutz D.</name></creator><creator><name>Momcheva I.G.,Nelson E.J.</name></creator><creator><name>Saglia R.P.</name></creator><creator><name>Seitz S.</name></creator><creator><name>Tadaki K.</name></creator><date role="Updated">2018-05-14T09:36:17Z</date><date role="Created">2018-03-08T15:33:02Z</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>infrared-sources</subject><subject>redshifted</subject><subject>galaxy-kinematics</subject><subject>stellar-masses</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><description>We investigate the stellar mass and baryonic mass Tully-Fisher relations (TFRs) of massive star-forming disk galaxies at redshift z~2.3 and z~0.9 as part of the KMOS^3D^ integral field spectroscopy survey. Our spatially resolved data allow reliable modeling of individual galaxies, including the effect of pressure support on the inferred gravitational potential. At fixed circular velocity, we find higher baryonic masses and similar stellar masses at z~2.3 as compared to z~0.9. Together with the decreasing gas-to-stellar mass ratios with decreasing redshift, this implies that the contribution of dark matter to the dynamical mass on the galaxy scale increases toward lower redshift. A comparison to local relations reveals a negative evolution of the stellar and baryonic TFR zero points from z=0 to z~0.9, no evolution of the stellar TFR zero point from z~0.9 to z~2.3, and a positive evolution of the baryonic TFR zero point from z~0.9 to z~2.3. We discuss a toy model of disk galaxy evolution to explain the observed nonmonotonic TFR evolution, taking into account the empirically motivated redshift dependencies of galactic gas fractions and the relative amount of baryons to dark matter on galaxy and halo scales.</description><source format="bibcode">2017ApJ...842..121U</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/842/121</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/324/877">J/A+A/324/877 : Spiral &amp; irregular galaxies HI properties (Broeils+, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/114/2402">J/AJ/114/2402 : Rotation curves of early-type galaxies (Courteau+, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/633/844">J/ApJ/633/844 : Stellar mass in disk-dominated galaxies (Pizagno+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/455/107">J/A+A/455/107 : 3D spectroscopy with VLT/GIRAFFE (Flores+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/653/1027">J/ApJ/653/1027 : TKRS/GOODS-N Field galaxies (Weiner+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/134/945">J/AJ/134/945 : Tully-Fisher relation for SDSS galaxies (Pizagno+, 2007)</relatedResource><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/706/1364">J/ApJ/706/1364 : SINS survey of high-redshift gal. 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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>logM*</name><description>[9.5/11.5] log stellar mass</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logMb</name><description>[9.8/11.7] log baryonic mass</description><unit>log(solMass)</unit><ucd>phys.mass</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Vcirc</name><description>[111.6/476.1] Maximum modeled circular velocity</description><unit>km/s</unit><ucd>phys.veloc</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>sigma0</name><description>[1/159] Modeled intrinsic velocity dispersion</description><unit>km/s</unit><ucd>phys.veloc.dispersion;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>