J/ApJS/244/40ivo://CDS.VizieR/J/ApJS/244/40doi:10.26093/cds/vizier.22440040CDSLiu D.Lang P.Magnelli B.Schinnerer E.Leslie S.Fudamoto Y.,Bondi M.Groves B.Jimenez-Andrade E.Harrington K.Karim A.,Oesch P.A.Sargent M.Vardoulaki E.Badescu T.Moser L.Bertoldi F.,Battisti A.da Cunha E.Zavala J.Vaccari M.Davidzon I.Riechers D.,Aravena M.2022-08-09T14:21:42Z2020-05-12T09:11:29ZCDS support team

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

cds-question@unistra.frgalaxiescatalogsmillimeter-astronomyphotometrysubmillimeter-astronomyredshiftedThe rich information on (sub)millimeter dust continuum emission from distant galaxies in the public Atacama Large Millimeter/submillimeter Array (ALMA) archive is contained in thousands of inhomogeneous observations from individual PI-led programs. To increase the usability of these data for studies deepening our understanding of galaxy evolution, we have developed automated mining pipelines for the ALMA archive in the COSMOS field (A3COSMOS) that efficiently exploit the available information for large numbers of galaxies across cosmic time and keep the data products in sync with the increasing public ALMA archive: (a) a dedicated ALMA continuum imaging pipeline, (b) two complementary photometry pipelines for both blind source extraction and prior source fitting, (c) a counterpart association pipeline utilizing the multiwavelength data available (including quality assessment based on machine-learning techniques), (d) an assessment of potential (sub)millimeter line contribution to the measured ALMA continuum, and (e) extensive simulations to provide statistical corrections to biases and uncertainties in the ALMA continuum measurements. Application of these tools yields photometry catalogs with ~1000 (sub)millimeter detections (spurious fraction ~8%-12%) from over 1500 individual ALMA continuum images. Combined with ancillary photometric and redshift catalogs and the above quality assessments, we provide robust information on redshift, stellar mass, and star formation rate for ~700 galaxies at redshifts 0.5-6 in the COSMOS field (with undetermined selection function). The ALMA photometric measurements and galaxy properties are released publicly within our blind extraction, prior fitting, and galaxy property catalogs, plus the images.2019ApJS..244...40Lhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/244/40CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toII/284 : COSMOS Multi-Wavelength Photometry Catalog (Capak+, 2007)VIII/103 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)VIII/95 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)J/A+A/403/857 : VLA-VIRMOS Deep Field (Bondi+, 2003)J/AJ/126/1607 : IRAS Revised Bright Galaxy Sample (Sanders+, 2003)J/ApJS/172/70 : zCOSMOS-bright catalog (Lilly+, 2007)J/AJ/136/2782 : Star formation efficiency in nearby galaxies (Leroy+, 2008)J/AJ/136/2563 : HI Nearby Galaxy Survey, THINGS (Walter+, 2008)J/ApJS/184/158 : Chandra COSMOS survey I. (Elvis+, 2009)J/ApJS/184/218 : The zCOSMOS 10k-bright spectroscopic sample (Lilly+, 2009)J/ApJS/188/384 : The VLA-COSMOS survey. IV. (Schinnerer+, 2010)J/MNRAS/415/3831 : AzTEC/ASTE source catalogue (Aretxaga+, 2011)J/A+A/533/A119 : GOODS-Herschel North and South catalogs (Elbaz+, 2011)J/MNRAS/411/102 : AzTEC/ASTE 1.1mm observations in the ADF-S (Hatsukade+ 2011)J/A+A/532/A90 : PACS Evolutionary Probe (PEP-DR1) catalogs (Lutz+, 2011)J/ApJ/742/61 : Phot. redshift of AGNs from XMM- and C-COSMOS (Salvato+ 2011)J/ApJ/761/140 : Spectroscopy of Herschel-SPIRE galaxies (Casey+, 2012)J/ApJS/201/30 : The Chandra COSMOS survey. III. (Civano+, 2012)J/A+A/544/A156 : UltraVISTA Catalogue Release DR1 (McCracken+, 2012)J/A+A/551/A100 : Panchromatic SED of Herschel sources (Berta+, 2013)J/A+A/556/A55 : Multi-color phot. of star-forming galaxies (Ilbert+, 2013)J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013)J/ApJ/768/74 : PHIBSS: CO obs. of star-forming galaxies (Tacconi+, 2013)J/MNRAS/441/1017 : Multiwavelength photometry of 34 galaxies (Rowlands+, 2014)J/ApJ/783/84 : ALMA obs. in 107 galaxies at z=0.2-2.5 (Scoville+, 2014)J/A+A/578/A11 : Spectrum of QSO XMMC 2028 (Brusa+, 2015)J/ApJ/812/43 : ALMA 870um obs. of HerMES galaxies (Bussmann+, 2015)J/ApJS/218/33 : Spitzer-CANDELS catalog within 5 deep fields (Ashby+, 2015)J/ApJS/219/8 : SFR for WISE + SDSS spectroscopic galaxies (Chang+, 2015)J/A+A/575/A40 : [OII] luminosity function (Comparat+, 2015)J/ApJ/806/110 : ALESS survey: SMGs in the ECDF-S data (da Cunha+, 2015)J/ApJS/220/12 : FMOS-COSMOS survey III. 0.7<z<2.5 galaxies (Silverman+, 2015)J/ApJ/819/62 : The COSMOS-Legacy Survey (CLS) catalog (Civano+, 2016)J/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016)J/ApJ/817/34 : C-COSMOS Legacy sources multiwavelength cat. (Marchesi+, 2016)J/ApJ/828/21 : ZFIRE v1.0 data release (Nanayakkara+, 2016)J/ApJ/820/83 : ALMA galaxy data in the COSMOS survey field (Scoville+, 2016)J/ApJ/819/69 : [NII]205um emission in local luminous IR gal. (Zhao+, 2016)J/ApJ/830/51 : FourStar galaxy evolution survey (ZFOURGE) (Straatman+, 2016)J/ApJ/850/83 : DANCING-ALMA. I. submm/mm continuum sources (Fujimoto+, 2017)J/MNRAS/465/1789 : SCUBA-2 Cosmology Legacy Survey (Geach+, 2017)J/ApJ/841/111 : C3R2 survey: high-confidence z from DR1 (Masters+, 2017)J/ApJ/839/58 : ALMA submm galaxies multi-wavelength data (Simpson+, 2017)J/A+A/602/A1 : VLA-COSMOS 3 GHz Large Project (Smolcic+, 2017)J/A+A/600/A110 : VIMOS Ultra Deep Survey (VUDS) DR1 (Tasca+, 2017)J/ApJS/237/39 : Spitzer survey of UltraVISTA deep Stripes (Ashby+, 2018)J/ApJ/858/77 : DEIMOS 10K spectrosc. survey in COSMOS field (Hasinger+, 2018)J/ApJ/853/172 : "Super-deblended" dust emission in galaxies. I. (Liu+, 2018)J/A+A/625/A114 : Star-forming gal. over 0.35<z<2.25 (Jimenez-Andrade+, 2019)http://sites.google.com/view/a3cosmos/ : A_3_COSMOS home pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/244/40https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/244/40http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/244/40https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/244/40https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/244/40http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/244/40GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/244/40/blind (The "blind"-extraction photometry catalog; all sources with S/N_peak>5.40 in the ALMA continuum data (see Section 2.2))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/244/40/blind?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/244/40/blind?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/244/40/blind?GETtext/xml+votable180.050000true150.08968540222.59069850840.005555555555555556Cone search capability for table J/ApJS/244/40/prior (The "prior"-fitting photometry catalog; known sources in deep optical/near-infrared/radio catalogs which have S/N_peak>4.35 in the ALMA continuum data (see Section 2.4))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/244/40/prior?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/244/40/prior?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/244/40/prior?GETtext/xml+votable180.050000true150.08648952.58923140.005555555555555556Cone search capability for table J/ApJS/244/40/catalog (*A3COSMOS final galaxy catalog (see Section 4))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/244/40/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/244/40/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/244/40/catalog?GETtext/xml+votable180.050000true149.65836021.53803730.005555555555555556Associated datahttps://cdsarc.cds.unistra.fr/assocdata/?obs_collection=J/ApJS/244/405/6814 6/27245 27247 27344https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/244/40?format=asciiMillimeterdefaultJ/ApJS/244/40/blindThe "blind"-extraction photometry catalog; all sources with S/N_peak>5.40 in the ALMA continuum data (see Section 2.2)Fluxc[0.04/52.4] The fitted total flux with Gaussian source models, corrected for flux bias and PBA (Total_flux_pbcor)mJyphot.flux.density;em.radiofloats_Fluxc[0.009/5] Fluxc error but estimated from our own simulation statistics (E_Total_flux_sim_pbcor)mJystat.error;phot.flux.densityfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right ascension of the ALMA emission (J2000)degpos.eq.ra;meta.mainDEJ2000Declination of the ALMA emission (J2000)degpos.eq.dec;meta.maine_Fluxc[0.01/6.2] Fluxc uncertainty (E_Total_flux_pbcor) (G1)mJystat.errorfloatPbcor[0.2/1] Primary beam attenuation (PBA) factorinstr.paramfloatBeam[8.6/64.6] ALMA 12m antenna's primary beam FWHM size at the observing frequency (Primary_beam)arcsecphys.angSize;em.radio.20-100MHz;instr.beamfloatFPk[0.02/27.6] Fitted ALMA continuum emission's peak flux, uncorrected for PBA (Peak_flux)mJy/beamphot.flux.density;em.radiofloatrms[0.005/1.8] Pixel rms noise in the continuum image (RMS_noise)mJy/beamstat.stdev;instr.det.noise;instr.pixelfloatFreq[90.2/671.5] Observing frequency, i.e., the center frequency of all collapsed spectral windows (Obs_frequency)GHzem.freqfloatlambda[446.4/3323.7] Observing wavelength =(2.99792458x10^5^)/Freq (Obs_wavelength)umem.wldoubleFWHMa[0.1/3.9] Synthesized beam's major-axis FWHM size (Maj_beam)arcsecphys.angSize.smajAxisfloatFWHMb[0.09/2.6] Synthesized beam's minor axis FWHM size (Min_beam)arcsecphys.angSize;instr.beamfloatPA[-90/90] Synthesized beam's position angle; zero means to the north (PA_beam)degpos.posAng;instr.beamfloatfitsDownload the FITS filemeta.ref.urlcharFileNameName of the image FITS file in subdirectory fits (Image_file)meta.id;meta.fitscharMult[MS] Flag= S (or M) means that the source is fitted with single (or multiple) Gaussian component(s) (Flag_multi)meta.code.error;pos.cartesian.y;meta.modelledcharFlag[0/1] 0=reliable flux (Flag_inconsistent_flux) (G2)meta.code.errorintJ/ApJS/244/40/priorThe "prior"-fitting photometry catalog; known sources in deep optical/near-infrared/radio catalogs which have S/N_peak>4.35 in the ALMA continuum data (see Section 2.4)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRDisplay the star formation data for this robust galaxy (link to the final catalog)meta.ref.urlcharIDA3COSMOS master catalog identification number (G3)meta.id;meta.mainintprimaryOIDID number in "Ref" (ID_PriorCat)meta.id.crossintRAJ2000Right ascension of the ALMA emission (J2000)degpos.eq.ra;meta.mainDEJ2000Declination of the ALMA emission (J2000)degpos.eq.dec;meta.mainFluxc[0.04/55.6] The fitted total flux with Gaussian source models, corrected for flux bias and PBA (Total_flux_pbcor)mJyphot.flux.density;em.radiofloate_Fluxc[0.01/6.2] Fluxc uncertainty (E_Total_flux_pbcor) (G1)mJystat.errorfloats_Fluxc[0.01/5.7] Fluxc error but estimated from our own simulation statistics (E_Total_flux_sim_pbcor)mJystat.error;phot.flux.densityfloatPbcor[0.2/1] Primary beam attenuation (PBA) factorinstr.paramfloatBeam[8.6/64.6] ALMA 12m antenna's primary beam FWHM size at the observing frequency (Primary_beam)arcsecphys.angSize;em.radio.20-100MHz;instr.beamfloatFPk[0.02/27.6] Fitted ALMA continuum emission's peak flux, uncorrected for PBA (Peak_flux)mJy/beamphot.flux.density;em.radiofloatrms[0.005/1.8] Pixel rms noise in the continuum image (RMS_noise)mJy/beamstat.stdev;instr.det.noise;instr.pixelfloatFreq[90.1/671.5] Observing frequency, i.e., the center frequency of all collapsed spectral windows (Obs_frequency)GHzem.freqfloatlambda[446.4/3325.5] Observing wavelength =(2.99792458x10^5^)/Freq (Obs_wavelength)umem.wldoubleFWHMa[0.1/3.9] Synthesized beam's major-axis FWHM size (Maj_beam)arcsecphys.angSize.smajAxisfloatFWHMb[0.09/2.6] Synthesized beam's minor axis FWHM size (Min_beam)arcsecphys.angSize;instr.beamfloatPA[-90/90] Synthesized beam's position angle; zero means to the north (PA_beam)degpos.posAng;instr.beamfloatfitsDownload the FITS filemeta.ref.urlcharFileNameName of the image FITS file in subdirectory fits (Image_file)meta.id;meta.fitscharChi2[0.01/48.2] The reduced {chi}^2^ of galfit prior source fitting, measured from the residual image for each source with an aperture of 1.0" in diameter (Galfit_reduced_chi_square)stat.fitfloatBound[0/1] Flag=1 means that the fitted source major-axis FWHM size reaches the upper boundary of 3.0" and should be used with caution (Flag_size_upper_boundary)meta.codeintFlag[0/1] 0=Reliable flux (Flag_inconsistent_flux) (G2)meta.code.errorintCPA[0/1] Unreliable counterpart outlier flag; see Section 4.2 (Flag_outlier_CPA)meta.codeintSED[0/1] SED-excess outlier flag; see Section 4.4 (Flag_outlier_SED)meta.codeintSMUVSDisplay data from Ashby+, 2018, J/ApJS/237/39 within 0.5"meta.ref.urlintnullableL16Display the COSMOS2015 data (Laigle+, 2016, J/ApJS/224/24) for this sourcemeta.ref.urlcharRefThe reference of the prior catalog in which the source is first included (Ref_ID_PriorCat) (1)meta.ref;pos.frame;meta.tablecharJ/ApJS/244/40/catalog*A3COSMOS final galaxy catalog (see Section 4)SimbadNameSimbad column added by the CDSmeta.idcharnullableMstar[2.7e+9/8.4e+12] Stellar mass from our SED fitting (M_star) (3)solMassphys.massdoubleID[168767/1389517] A3COSMOS master catalog identification number (G3)meta.id;meta.mainintsSFR[0.1/35] Specific SFR from SFH; SFR/Mstarx10^9^Gyr**-1phys.SFRfloatr_zReference for z (1)meta.ref;pos.framecharzPriorPrior redshifts in the literature (z_prior)src.redshift;pos.heliocentricr_zPriorReferences of zPrior (Ref_z_prior) (2)meta.ref;pos.framecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right ascension of the ALMA emission (J2000)degpos.eq.ra;meta.mainDEJ2000Declination of the ALMA emission (J2000)degpos.eq.dec;meta.mainz[0.3/7.3] SED best-fit redshift from the list of prior redshiftssrc.redshiftfloatf_zp: photometric or s: spectroscopicmeta.codecharq_z[1/212]? Quality flag "Qz" for dzLiu or S17meta.code.qual;src.redshiftintnullableLdust[9.3e+10/3.9e+13] Infrared 8-1000u luminosity from dust (L_dust) (3)solLumphys.luminosity;em.IRdoubleSFR[9.3/3890.5] SFR integrated from SFH (3)solMass/yrphys.SFRdouble