J/A+A/643/A2ivo://CDS.VizieR/J/A+A/643/A2doi:10.26093/cds/vizier.36430002CDSBethermin M.Fudamoto Y.Ginolfi M.Loiacono F.Khusanova Y.,Capak P.L.Cassata P.Faisst A.Le Fevre O.Schaerer D.,Silverman J.D.Yan L.Amorin R.Bardelli S.Boquien M.Cimatti A.,Davidzon I.Dessauges-Zavadsky M.Fujimoto S.Gruppioni C.Hathi N.P.,Ibar E.Jones G.C.Koekemoer A.M.Lagache G.Lemaux B.C.Moreau C.,Oesch P.A.Pozzi F.Riechers D.A.Talia M.Toft S.Vallini L.,Vergani D.Zamorani G.Zucca E.2022-04-07T08:04:48Z2020-10-27T07:25:27ZCDS support team

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

cds-question@unistra.frsurveysinterstellar-mediumgalaxiescatalogsredshiftedmillimeter-astronomysubmillimeter-astronomyultraviolet-astronomyThe ALPINE-ALMA large program targets the [CII] 158um line and the far-infrared continuum in 118 spectroscopically confirmed star-forming galaxies between z=4.4 and z=5.9. It represents the first large [CII] statistical sample built in this redshift range. We present details of the data processing and the construction of the catalogs. We detected 23 of our targets in the continuum. To derive accurate infrared luminosities and obscured star formation rates, we measured the conversion factor from the ALMA 158um rest-frame dust continuum luminosity to the total infrared luminosity (LIR) after constraining the dust spectral energy distribution by stacking a photometric sample similar to ALPINE in ancillary single-dish far-infrared data. We found that our continuum detections have a median LIR of 4.4x10^11^L_{sun}_. We also detected 57 additional continuum sources in our ALMA pointings. They are at lower redshift than the ALPINE targets, with a mean photometric redshift of 2.5+/-0.2. We measured the 850um number counts between 0.35 and 3.5mJy, improving the current interferometric constraints in this flux density range. We found a slope break in the number counts around 3mJy with a shallower slope below this value. More than 40% of the cosmic infrared background is emitted by sources brighter than 0.35mJy. Finally, we detected the [CII] line in 75 of our targets. Their median [CII] luminosity is 4.8x108L_{sun}_ and their median full width at half maximum is 252km/s. After measuring the mean obscured SFR in various [CII] luminosity bins by stacking ALPINE continuum data, we find a good agreement between our data and the local and predicted SFR-L[CII] relations of De Looze et al. (2014A&A...568A..62D) and Lagache et al. (2018A&A...609A.130L).2020A&A...643A...2Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/643/A2CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/643/A2https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/643/A2http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/643/A2https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/643/A2https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/643/A2http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/643/A2GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/643/A2/catalog (ALPINE DR1 merged catalog)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/643/A2/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/643/A2/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/643/A2/catalog?GETtext/xml+votable180.050000true53.2251-27.833560.0055555555555555566/27256 27258-27259 35935https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/643/A2?format=asciiUVMillimeterdefaultJ/A+A/643/A2/catalogALPINE DR1 merged catalogrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintFCIICII line fluxJy.km/sphot.flux.density;spect.linefloatLCIICII luminositysolLumphys.luminositydoublel_EWLya[<] Limit flag on EWLyameta.code.errorchare_betamedComb[]? Error on beta_med_comb (1sigma) (lower value)stat.errordoublenullableSimbadNameSimbad column added by the CDSmeta.idcharnullablee_FCII? 1-sigma uncertainty on the CII line fluxJy.km/sstat.errorfloatnullablel_LCII[<] Limit flag on LCII, if "<" LCII is 3-sigma secure upper limit if non detectionmeta.code.errorchare_LCII? 1-sigma uncertainty on LCII,solLumstat.errordoublenullablezCII? CII redshiftsrc.redshift;pos.heliocentricfloatnullablee_zCII? Uncertainties on the CII redshiftstat.errorfloatnullableCIIFWHM? FWHM of the CII linekm/sspect.line.widthintnullablee_CIIFWHM? Uncertainty on CII_FWHMkm/sstat.errorintnullableSNRCII? CII SNR measured in the mom-0 mapstat.snrfloatnullablef_CII[0/1] Flag indicating a complex [CII] photometry (1)meta.codeintl_Scont[<] Limit flag on Scont, if "<" Scont is 3-sigma secure upper limit if non detectionmeta.code.errorcharScont~155-um continuum fluxmJyphot.flux.density;spect.continuumfloate_Scont? 1-sigma uncertainty on ScontmJystat.errorfloatnullablel_L155[<] Limit flag on L155, if "<" L155 is 3-sigma secure upper limit if non detectionmeta.code.errorcharL155~155-um continuum monochromatic luminosity (Lsun, nuLnu unit)solLumphys.luminosity;spect.continuumdoublee_L155? 1-sigma uncertainty on L155,solLumstat.errordoublenullablel_LIR[<] Limit flag on LIR, if "<" LIR is 3-sigma secure upper limit if non detectionmeta.code.errorcharLIRIntegrated 8-1000 micron luminosity (Lsun, nuLnu unit)solLumphys.luminosity;em.IRdoublee_LIR? 1-sigma uncertainty on LIR (Lsun, nuLnu unit)solLumstat.errordoublenullablerestFreq? Effective rest-frame frequency at which the continuum is measuredGHzem.freqfloatnullableSNRcont? Peak SNR in the continuum mapstat.snr;stat.maxfloatnullablef_cont[0/1] flag indicating a complex continuum photometry (1)meta.codeintMkinClass[1/5]? Morpho kinematic class (2)src.morph.typeintnullableCIIsizeCII size [kpc]kpcphys.angSizedoublee_CIIsize1-sigma uncertainty on the CII sizekpcstat.error;pos.distance;phys.sizedoublef_CIIsize[0/1]? 0 if reliablemeta.codeintnullableRAJ2000Right ascension (J2000) from either the COSMOS or 3D-HST catalogdegpos.eq.ra;meta.maindRAConstant shift (to be added to RA) in R.A. due to astrometric offset (3)maspos.eq.ra;arith.diffdoubleDEJ2000Declination (J2000) from either the COSMOS or 3D-HST catalogdegpos.eq.dec;meta.maindDEConstant shift (to be added to DEC) in decl. due to astrometric offset (3)maspos.eq.dec;arith.diffdoubleField[1/2] Field name, 1 = ECDFS or 2 = COSMOSmeta.codeintSelSelection Original selection (4)meta.codecharzorigOriginal redshift used for initial selection (5)src.redshift;pos.heliocentricfloatzCII2? Redshift determined from FIR [CII] emission lines (see details in paper) Is -99 if [CII] is not detected at S/N>3.5src.redshift;pos.heliocentricdoublenullableNameALPINE Unique name for each galaxymeta.id;meta.maincharMclass? Morpho-kinematic classes from Le Fevre et al. (2019, arXiv:1910.09517) (6)src.class.luminosityintnullablehastwin[0/1] A flag set to 1 of for a galaxy has been observed by Keck/DEIMOS and VUDS (two spectra available), If false, the flag is set to 0meta.codeintzLya? Redshift determined from peak of Ly{alpha} emission (7)src.redshift;pos.heliocentricdoublenullableEWLyaObserver-frame Ly{alpha} emission equivalent (7)spect.line.eqWidthdoublee_EWLya[]? 1{sigma} uncertainty on observer-frame Ly{alpha} emission equivalent (8)stat.errordoublenullableFLya? Ly{alpha} emission flux (7)mW.m**-2phot.flux;em.UVdoublenullablef_specpro[1/3]? Visual flag for reliability of absorption redshift measurements (9)meta.codeintnullableziswind? Redshift determined from IS+wind absorption lines (see Section 2.4)src.redshift;pos.heliocentricdoublenullablee_ziswind? Error on ziswind (lower value, 95% percentile)stat.errordoublenullableE_ziswind? Error on ziswind (upper value, 95% percentile)stat.error;stat.maxdoublenullableo_ziswind? Number of lines used for IS+wind redshift measurement (10)meta.numberintnullablezwind? Redshift determined from wind absorption lines (see Section 2.4)src.redshift;pos.heliocentricdoublenullablee_zwind? Error on zwind (lower value, 95% percentile)stat.errordoublenullableE_zwind? Error on zwind (upper value, 95% percentile)stat.error;stat.maxdoublenullableo_zwind? Number of lines used for wind redshift measurement (11)meta.numberintnullableIDphotcatID in the photometric catalogs, 3D-HST catalog for galaxies in ECDFS and the COSMOS2015 catalog for galaxies in COSMOSmeta.idintchi2chi^2^ value given by the LePhare fitstat.fit.chi2;stat.fit.param;meta.modelleddoubleNbandNumber of bands used for SED fittingmeta.numberintE(B-V)? E(B-V) derived from SED fittingmagphot.color.excessdoublenullablelogAge? Logarithmic agelog(yr)time.agedoublenullablee_logAge? Error on logAge (1sigma) (lower value)log(yr)stat.error;time.agedoublenullableE_logAge? Error on logAge (1sigma) (upper value)log(yr)stat.error;stat.maxdoublenullablelogMstar? Logarithmic stellar masslog(solMass)phys.massdoublenullablee_logMstar? Error on logMstar (1sigma) (lower value)log(solMass)stat.errordoublenullableE_logMstar? Error on logMstar (1sigma) (upper value)log(solMass)stat.error;stat.maxdoublenullablelogSFRSED? Logarithmic star formation rate from SEDlog(solMass.yr**-1)phys.SFRdoublenullablee_logSFRSED? Error on logSFRSED (1sigma) (lower value)log(solMass.yr**-1)stat.errordoublenullableE_logSFRSED? Error on logSFRSED (1sigma) (upper value)log(solMass.yr**-1)stat.error;stat.maxdoublenullablelogsSFR? Logarithmic specific star formation ratelog(yr**-1)phys.SFRdoublenullablee_logsSFR[]? Error on logsSFR (1sigma) (lower value)log(yr**-1)stat.errordoublenullableE_logsSFR[]? Error on logsSFR (1sigma) (upper value)log(yr**-1)stat.error;stat.maxdoublenullableUVMAG? Absolute rest-frame UV magnitude measured in the GALEX FUV filter (corresponding approximately to rest-frame 1500{AA}magphys.magAbsfloatnullablee_UVMAG[]? Error on UVMAG (1sigma) (lower value)magstat.errorfloatnullableE_UVMAG[]? Error on UVMAG (1sigma) (upper value)magstat.error;stat.maxfloatnullablebetamedC? UV slope measured assuming Calzetti (2000ApJ...533..682C) dustspect.indexdoublenullablee_betamedC[]? Error on beta_med_calz (1sigma) (lower value)stat.errordoublenullableE_betamedC[]? Error on beta_med_calz (1sigma) (upper value)stat.error;stat.maxdoublenullablebetamedSMC? UV slope measured assuming SMC dustspect.indexdoublenullablee_betamedSMC[]? Error on beta_med_smc (1sigma) (lower value)stat.errordoublenullableE_betamedSMC[]? Error on beta_med_smc (1sigma) (upper value)stat.error;stat.maxdoublenullablebetamedComb? UV slope measured by marginalizing over Calzetti (2000ApJ...533..682C) and SMC dustspect.indexdoublenullableE_betamedComb[]? Error on beta_med_comb (1sigma) (upper value)stat.error;stat.maxdoublenullableSpitzer[0/2] Spitzer photometry contamination flag (12)meta.code.error;photintEWHamed? Rest-frame H{alpha} equivalent width assuming Calzetti et al. (2000ApJ...533..682C) dust attenuation and f=0.440.1nmspect.line.eqWidthdoublenullablee_EWHamed? Error on EWHamed (lower value)0.1nmstat.errordoublenullableE_EWHamed? Error on eWHamed (upper value)0.1nmstat.error;stat.maxdoublenullablelogHaLummed? Logarithmic H{alpha} luminosity assuming Calzetti et al. (2000ApJ...533..682C) dust attenuation and f=0.44log(1e-07W)phys.luminosity;em.line.Halphadoublenullablee_logHaLummed? Error on logHaLummed (lower value)log(1e-07W)stat.errordoublenullableE_logHaLummed? Error on logHaLummed (upper value)log(1e-07W)stat.error;stat.maxdoublenullablelogSFRHamed? Logarithmic star formation rate based on H{alpha} luminosity (13)phys.SFRdoublenullablee_logSFRHamed[]? Error on logSFRHamed (lower value)stat.errordoublenullableE_logSFRHamed[]? Error on logSFRHamed (upper value)stat.error;stat.maxdoublenullablel_FCII[<] Limit flag on FCII, if "<" FCII is 3-sigma secure upper limit if non detectionmeta.code.errorchar