J/MNRAS/482/2166ivo://CDS.VizieR/J/MNRAS/482/2166doi:10.26093/cds/vizier.74822166CDSTiley A.L.Bureau M.Cortese L.Harrison C.M.Johnson H.L.Stott J.P.,Swinbank A.M.Smail I.Sobral D.Bunker A.J.Glazebrook K.Bower R.G.,Obreschkow D.Bryant J.J.Jarvis M.J.Bland-Hawthorn J.Magdis G.,Medling A.M.Sweet S.M.Tonini C.Turner O.J.Sharples R.M.,Croom S.M.Goodwin M.Konstantopoulos I.S.Lorente N.P.F.,Lawrence J.S.Mould J.Owers M.S.Richards S.N.2024-08-19T20:14:46Z2022-08-01T15:25:32ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgalaxiesredshiftedWe construct Tully-Fisher relations (TFRs), from large samples of galaxies with spatially resolved H{alpha} emission maps from the K-band Multi-Object Spectrograph (KMOS) Redshift One Spectroscopic Survey (KROSS) at z~1. We compare these to data from the Sydney-Australian-Astronomical-Observatory Multi-object Integral-Field Spectrograph (SAMI) Galaxy Survey at z~0. We stringently match the data quality of the latter to the former, and apply identical analysis methods and sub-sample selection criteria to both to conduct a direct comparison of the absolute K-band magnitude and stellar mass TFRs at z~1 and 0. We find that matching the quality of the SAMI data to that of KROSS results in TFRs that differ significantly in slope, zero-point, and (sometimes) scatter in comparison to the corresponding original SAMI relations. These differences are in every case as large as or larger than the differences between the KROSS z~1 and matched SAMI z~0 relations. Accounting for these differences, we compare the TFRs at z~1 and 0. For disc-like, star-forming galaxies we find no significant difference in the TFR zero-points between the two epochs. This suggests the growth of stellar mass and dark matter in these types of galaxies is intimately linked over this ~8Gyr period.2019MNRAS.482.2166Thttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/482/2166CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/MNRAS/467/1965 : KMOS Redshift One Spectroscopic Survey (Harrison+, 2017)J/MNRAS/474/5076 : KMOS Redshift One Spectroscopic Survey (Johnson+, 2018)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/482/2166https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/482/2166http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/482/2166https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/482/2166https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/482/2166http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/482/2166GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/MNRAS/482/2166/tablea1The derived properties used to construct the KROSS, original SAMI, and matched SAMI TFRs for the rot-dom and disky sub-samplesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSurveyThe source survey for the galaxy (KROSS, SAMI_matched or SAMI_original)meta.notecharIDThe object ID for the corresponding survey for KROSS survey, KROSS NNNNNN in Simbadmeta.id;meta.mainintf_ID[0/1] Flag indicating to which sub-sample(s) the galaxy belongs (1)meta.codeintlogv2.2Intrinsic rotation velocity (2)log(km.s**-1)phys.veloc.rotatdoublee_logv2.2Error on logv2.2 (2)log(km.s**-1)stat.errordoublelogMstarThe stellar mass derived via SED fitting with LEPHARE (3)log(solMass)phys.massdoublee_logMstarError on logMstar (3)log(solMass)stat.errorfloatKMAGAbsolute K-band magnitude in the Vega systemmagphot.magfloate_KMAGError on KMAGmagstat.errorfloat