J/A+A/685/A48ivo://CDS.VizieR/J/A+A/685/A48doi:10.26093/cds/vizier.36850048CDSHuertas-Company M.Iyer K.G.Angeloudi E.Bagley M.B.Finkelstein S.L.,Kartaltepe J.McGrath E.J.Sarmiento R.Vega-Ferrero J.Arrabal Haro P.,Behroozi P.Buitrago F.Cheng Y.Costantin L.Dekel A.Dickinson M.,Elbaz D.Grogin N.A.Hathi N.P.Holwerda B.W.Koekemoer A.M.,Lucas R.A.Papovich C.Perez-Gonzalez P.G.Pirzkal N.Seille L-M.,de la Vega A.Wuyts S.Yang G.Yung L.Y.A.2024-11-29T20:02:29Z2024-05-03T09:34:43ZCDS support team

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

cds-question@unistra.frgalaxiesinfrared-photometrygalaxy-classification-systemsThe James Webb Space Telescope's (JWST's) unprecedented combination of sensitivity, spatial resolution, and infrared coverage has enabled a new era of galaxy morphology exploration across most of cosmic history. We analyze the near-infrared (NIR~0.8-1um) rest-frame morphologies of galaxies with log M*/M_{sun}_>9 in the redshift range of 0<z<6, compare with previous HST-based results and release the first JWST-based morphological catalog of ~20000 galaxies in the CEERS survey. We classified the galaxies in our sample into four main broad classes: spheroid, disk+spheroid, disk, and disturbed, based on imaging with four filters: F150W, F200W, F356W, and F444W. We used convolutional neural networks (CNNs) trained on HST/WFC3 labeled images and domain-adapted to JWST/NIRCam. We find that ~90% and ~75% of galaxies at z<3 have the same early and late and regular and irregular classification, respectively, in JWST and HST imaging when considering similar wavelengths. For small (large) and faint objects, JWST-based classifications tend to systematically present less bulge-dominated systems (peculiar galaxies) than HST-based ones, but the impact on the reported evolution of morphological fractions is less than ~10%. Using JWST-based morphologies at the same rest-frame wavelength (~0.8-1um), we confirm an increase in peculiar galaxies and a decrease in bulge-dominated galaxies with redshift, as reported in previous HST-based works, suggesting that the stellar mass distribution, in addition to light distribution, is more disturbed in the early universe. However, we find that undisturbed disk-like systems already dominate the high-mass end of the late-type galaxy population (log M*/M_{sun}_>10.5) at z~5, and bulge-dominated galaxies also exist at these early epochs, confirming a rich and evolved morphological diversity of galaxies ~1Gyr after the Big Bang. Finally, we find that the morphology-quenching relation is already in place for massive galaxies at z>3, with massive quiescent galaxies (logM*/M_{sun}_>10.5) being predominantly bulge-dominated.2024A&A...685A..48Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/685/A48CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/685/A48https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/685/A48http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/685/A48https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/685/A48https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/685/A48http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/685/A48GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/685/A48/catalog (JWST-based morphological catalog of ~20000 galaxies in the CEERS survey)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/685/A48/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/685/A48/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/685/A48/catalog?GETtext/xml+votable180.050000true214.983215560172452.95202329540260.0055555555555555566/11425https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/685/A48?format=asciiOpticalInfrareddefaultJ/A+A/685/A48/catalogJWST-based morphological catalog of ~20000 galaxies in the CEERS surveyrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintID[1/101783] Identification numbermeta.id;meta.mainintRAJ2000Right ascension (J2000) (RA)degpos.eq.ra;meta.mainindexedDEJ2000Declination (J2000) (DE)degpos.eq.dec;meta.mainindexedSF200WMean CNN output spheroid class in filter F200W (sph_f200w_mean)stat.fit.goodnessdoublee_SF200WStandard deviation of CNN output spheroid class in filter F200W (sph_f200w_std)stat.errordoubleDF200WMean CNN output disk class in filter F200W (disk_f200w_mean)stat.fit.goodnessdoublee_DF200WStandard deviation of CNN output disk class in filter F200W(disk_f200w_std)stat.errordoubleIF200WMean CNN output irregular class in filter F200W (irr_f200w_mean)stat.fit.goodnessdoublee_IF200WStandard deviation of CNN output irregular class in filter F200W (irr_f200w_std)stat.errordoubleBF200WMean CNN output bulge/disk class in filter F200W (bd_f200w_mean)stat.fit.goodnessdoublee_BF200WStandard deviation of CNN output bulge/disk class in filter F200W (bd_f200w_std)stat.errordoubleSF356WMean CNN output spheroid class in filter F356W (sph_f356w_mean)stat.fit.goodnessdoublee_SF356WStandard deviation of CNN output spheroid class in filter F356W (sph_f356w_std)stat.errordoubleDF356WMean CNN output disk class in filter F356W (disk_f356w_mean)stat.fit.goodnessdoublee_DF356WStandard deviation of CNN output disk class in filter F356W (disk_f356w_std)stat.errordoubleIF356WMean CNN output irregular class in filter F356W (irr_f356w_mean)stat.fit.goodnessdoublee_IF356WStandard deviation of CNN output irregular class in filter F356W (irr_f356w_std)stat.errordoubleBF356WMean CNN output bulge/disk class in filter F356W (bd_f356w_mean)stat.fit.goodnessdoublee_BF356WStandard deviation of CNN output bulge/disk class in filter F356W (bd_f356w_std)stat.errordoubleSF444WMean CNN output spheroid class in filter F444W (sph_f444w_mean)stat.fit.goodnessdoublee_SF444WStandard deviation of CNN output spheroid class in filter F444W (sph_f444w_std)stat.errordoubleDF444WMean CNN output disk class in filter F444W (disk_f444w_mean)stat.fit.goodnessdoublee_DF444WStandard deviation of CNN output disk class in filter F444W (disk_f444w_std)stat.errordoubleIF444WMean CNN output irregular class in filter F444W (irr_f444w_mean)stat.fit.goodnessdoublee_IF444WStandard deviation of CNN output irregular class in filter F444W (irr_f444w_std)stat.errordoubleBF444WMean CNN output bulge/disk class in filter F444W (bd_f444w_mean)stat.fit.goodnessdoublee_BF444WStandard deviation of CNN output bulge/disk class in filter F444W (bd_f444w_std)stat.errordoublefF356W[0/3] F356W morphology flag (morph_flag_f356w) (1)meta.codeintfF200W[0/3] F200W morphology flag (morph_flag_f200w) (1)meta.codeintfF444W[0/3] F444W morphology flag (morph_flag_f444w) (1)meta.codeintSF150WMean CNN output spheroid class in filter F150W (sph_f150w_mean)stat.fit.goodnessdoublee_SF150WStandard deviation of CNN output spheroid class in filter F150W (sph_f150w_std)stat.errordoubleDF150WMean CNN output disk class in filter F150W (disk_f150w_mean)stat.fit.goodnessdoublee_DF150WStandard deviation of CNN output disk class in filter F150W (disk_f150w_std)stat.errordoubleIF150WMean CNN output irregular class in filter F150W (irr_f150w_mean)stat.fit.goodnessdoublee_IF150WStandard deviation of CNN output irregular class in filter F150W (irr_f150w_std)stat.errordoubleBF150WMean CNN output bulge/disk class in filter F150W (bd_f150w_mean)stat.fit.goodnessdoublee_BF150WStandard deviation of CNN output bulge/disk class in filter F150W (bd_f150w_std)stat.errordoublefF150W[0/3] F150W morphology flag (morph_flag_f150w) (1)meta.codeint