J/ApJ/910/106ivo://CDS.VizieR/J/ApJ/910/106doi:10.26093/cds/vizier.19100106CDSJimenez-Andrade E.F.Murphy E.J.Heywood I.Smail I.Penner K.,Momjian E.Dickinson M.Armus L.Lazio T.J.W.2023-08-16T14:46:46Z2022-09-30T16:28:12ZCDS support team

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

cds-question@unistra.frradio-galaxiesultraviolet-astronomyvisible-astronomygalaxy-classification-systemsredshiftedsurveysTo investigate the growth history of galaxies, we measure the rest-frame radio, ultraviolet (UV), and optical sizes of 98 radio-selected, star-forming galaxies (SFGs) distributed over 0.3<=z<=3 with a median stellar mass of log(M_*_/M_{sun}_)~10.4. We compare the size of galaxy stellar disks, traced by rest-frame optical emission, relative to the overall extent of star formation activity that is traced by radio continuum emission. Galaxies in our sample are identified in three Hubble Frontier Fields: MACS J0416.1-2403, MACSJ0717.5+3745, and MACS J1149.5+2223. Radio continuum sizes are derived from 3 and 6GHz radio images (<=0.6" resolution, ~0.9{mu}Jy/beam noise level) from the Karl G. Jansky Very Large Array. Rest-frame UV and optical sizes are derived using observations from the Hubble Space Telescope and the Advanced Camera for Surveys and Wide Field Camera 3 instruments. We find no clear dependence between the 3GHz radio size and stellar mass of SFGs, which contrasts with the positive correlation between the UV/optical size and stellar mass of galaxies. Focusing on SFGs with log(M_*_/M_{sun}_)>10, we find that the radio/UV/optical emission tends to be more compact in galaxies with high star formation rates (>=100M_{sun}_/yr), suggesting that a central, compact starburst (and/or an active galactic nucleus) resides in the most luminous galaxies of our sample. We also find that the physical radio/UV/optical size of radio-selected SFGs with log(M_*_/M_{sun}_)>10 increases by a factor of 1.5-2 from z~3 to z~0.3, yet the radio emission remains two to three times more compact than that from the UV/optical. These findings indicate that these massive, radio-selected SFGs at 0.3<=z<=3 tend to harbor centrally enhanced star formation activity relative to their outer disks.2021ApJ...910..106Jhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/910/106CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toIX/45 : The Chandra Source Catalog, Release 1.1 (Evans+ 2012)IX/57 : The Chandra Source Catalog (CSC), Release 2.0 (Evans+, 2019)J/ApJ/378/65 : 8.4GHz observations of compact starbursts (Condon+ 1991)J/ApJ/533/611 : 1.4GHz survey in HDF region (Richards+, 2000)J/ApJ/554/803 : New VLA Sky Survey (NVSS) Cat of IRAS 2Jy Gal. (Yun+ 2001)J/ApJ/586/794 : Multiwavelength luminosities of galaxies (Bell, 2003)J/ApJS/155/271 : Chandra Deep Field-South: Opt. spectroscopy (Szokoly+, 2004)J/MNRAS/358/1159 : Radio sources in HDF and HFF (Muxlow+, 2005)J/ApJS/188/384 : The VLA-COSMOS survey. IV. (Schinnerer+, 2010)J/A+A/533/A119 : GOODS-Herschel North and South catalogs (Elbaz+, 2011)J/A+A/545/A141 : UV selected sources in the GOODS-S field (Buat+, 2012)J/ApJ/761/97 : Star Formation in Radio Survey (SFRS): 33GHz (Murphy+, 2012)J/MNRAS/436/3759 : ECDFS sources optical/IR counterparts (Bonzini+, 2013)J/A+A/553/A80 : Dust effects on phot. parameters in spirals (Pastrav+, 2013)J/MNRAS/443/1549 : MACSJ0416.1-2403 strong-lensing analysis (Jauzac+, 2014)J/MNRAS/444/268 : HST Frontier Fields clusters (Richard+, 2014)J/ApJS/219/15 : Morphologies of z=0-10 galaxies with HST (Shibuya+, 2015)J/ApJS/224/33 : CLASH-VLT: the FF cluster MACSJ0416.1-2403 (Balestra+, 2016)J/ApJ/822/78 : VLT/MUSE sp. obs. of MACS J1149.5+2223 (Grillo+, 2016)J/MNRAS/459/1626 : HST Frontier Fields Herschel sources (Rawle+, 2016)J/A+A/597/A41 : ALMA Frontier Fields Survey. I. (Gonzalez-Lopez+, 2017)J/MNRAS/471/210 : eMERGE Survey. I. VLA 5.5GHz sources (Guidetti+, 2017)J/A+A/602/A2 : VLA-COSMOS 3 GHz Large Project. II. (Smolcic+, 2017)J/A+A/602/A1 : VLA-COSMOS 3 GHz Large Project (Smolcic+, 2017)J/ApJ/856/67 : VLA 3GHz radio source cat. in Lockman Hole (Cotton+, 2018)J/ApJS/235/34 : Deep JVLA imaging of GOODS-N at 20cm (Owen, 2018)J/ApJ/875/80 : Faint radio sources in GOODS-N & -S. I. 5GHz (Gim+, 2019)J/A+A/625/A114 : Star-forming gal. over 0.35<z<2.25 (Jimenez-Andrade+, 2019)J/ApJ/901/74 : ALMA obs. of UDS & GOODS-S massive galaxies (Tadaki+, 2020)http://science.nrao.edu/science/surveys/vla-ff : NRAO VLA FF survey home pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/910/106https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/910/106http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/910/106https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/910/106https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/910/106http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/910/106GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/910/106/table2 (The radio/UV/optical size of 98 field (and 15 cluster) galaxies in the HFF)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/910/106/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/910/106/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/910/106/table2?GETtext/xml+votable180.050000true64.0085-24.08986110.0055555555555555566/6383 28448 34793 34796https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/910/106?format=asciiUVOpticalRadiodefaultJ/ApJ/910/106/table2The radio/UV/optical size of 98 field (and 15 cluster) galaxies in the HFFrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDGalaxy identifier from Heywood+, 2021, J/ApJ/910/105meta.id;meta.maincharf_ID[*] Flag on ID (1)meta.codecharz[0.18/4.43] Redshiftsrc.redshiftfloatn_zRedshift type (s=spectroscopic or p=photometric)meta.notecharmu[0.99/6.45] Lensing magnification factorstat.paramfloatlogM*[8.74/12.3] log stellar masslog(solMass)phys.massfloatlogSFR[-0.3/3.8] log total Star Formation Rate dDerived from 3GHz and far-UV emissionlog(solMass.yr**-1)phys.SFRfloate_logSFR[0.02/0.3] Uncertainty in logSFRlog(solMass.yr**-1)stat.error;phys.SFRfloatRUV[0.29/9.33]? Effective UV radiuskpcphys.size.radiusfloatnullablee_RUV[0.01/7.67]? Uncertainty in RUVkpcstat.errorfloatnullableROpt[1.2/8.01]? Effective optical radiuskpcphys.size.radiusfloatnullablee_ROpt[0/1.77]? Uncertainty in ROptkpcstat.errorfloatnullableR3GHz[0/4.98] Effective 3GHz radiuskpcphys.size.radiusfloate_R3GHz[0.04/2.03] Uncertainty in R3GHzkpcstat.errorfloatf_R3GHzReliably resolved at 3GHz flag (2)meta.codecharR6GHz[0/4.03]? Effective 6 GHz radiuskpcphys.size.radiusfloatnullablee_R6GHz[0.08/1.08]? Uncertainty in R6GHzkpcstat.errorfloatnullablef_R6GHzReliably resolved at 6GHz flag (2)meta.codecharEnvEnvironment flag (c=cluster or f=field)meta.codecharSimbadSimbad column added by the CDSmeta.ref.urlchar_RAPositions from names (right ascension part)degpos.eq.ra;meta.main_DEPositions from names (declination part)degpos.eq.dec;meta.main