J/ApJS/261/12ivo://CDS.VizieR/J/ApJS/261/12doi:10.26093/cds/vizier.22610012CDSPharo J.Guo Y.Calvo G.B.Carleton T.Faber S.M.Guhathakurta P.,Kassin S.A.Koo D.C.Lonergan J.Teppala T.Wang W.Yesuf H.M.,Bian F.Dave R.Forbes J.C.Keres D.Perez-Gonzalez P.Martin A.,Puleo A.J.Williams L.Winningham B.2022-12-16T22:21:54Z2022-10-05T13:59:16ZCDS support team

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

cds-question@unistra.frgalaxiesspectroscopyredshiftedhst-photometryline-intensitiesWe present a catalog of spectroscopically measured redshifts over 0<z<2 and emission-line fluxes for 1440 galaxies. The majority (~65%) of the galaxies come from the HALO7D survey, with the remainder from the DEEPwinds program. This catalog includes redshifts for 646 dwarf galaxies with log(M_*_/M_{sun}_)<9.5. Eight-hundred and ten catalog galaxies did not have previously published spectroscopic redshifts, including 454 dwarf galaxies. HALO7D used the DEIMOS spectrograph on the Keck II telescope to take very deep (up to 32hr exposure, with a median of ~7hr) optical spectroscopy in the COSMOS, EGS, GOODS-North, and GOODS-South CANDELS fields, and in some areas outside CANDELS. We compare our redshift results to existing spectroscopic and photometric redshifts in these fields, finding only a 1% rate of discrepancy with other spectroscopic redshifts. We measure a small increase in median photometric redshift error (from 1.0% to 1.3%) and catastrophic outlier rate (from 3.5% to 8%) with decreasing stellar mass. We obtained successful redshift fits for 75% of massive galaxies, and demonstrate a similar 70%-75% successful redshift measurement rate in 8.5<log(M_*_/M_{sun}_)<9.5 galaxies, suggesting similar survey sensitivity in this low-mass range. We describe the redshift, mass, and color-magnitude distributions of the catalog galaxies, finding HALO7D galaxies representative of CANDELS galaxies up to i-band magnitudes of 25.2022ApJS..261...12Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/261/12CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toII/284 : COSMOS Multi-Wavelength Photometry Catalog (Capak+, 2007)II/318 : GOODS Source Catalogs release r2.0z (Giavalisco+ 2008)J/AJ/127/3121 : TKRS catalog of GOODS-North Field (Wirth+, 2004)J/ApJ/690/1236 : COSMOS photometric redshift catalog (Ilbert+, 2009)J/ApJ/706/599 : H{alpha} and UV SFR in the local volume (Lee+, 2009)J/ApJS/193/13 : Spitzer/IRAC sources in the EGS I. SEDs (Barro+, 2011)J/ApJS/193/30 : UV-to-FIR analysis of sources in the EGS. II. (Barro+, 2011)J/ApJS/193/14 : DEEP3 Galaxy Redshift Survey: GOODS-N field (Cooper+, 2011)J/ApJS/203/24 : Structural param. of CANDELS galaxies (van der Wel+, 2012)J/ApJ/744/44 : H{alpha} and UV fluxes in nearby galaxies (Weisz+, 2012)J/ApJS/207/24 : GOODS-S CANDELS multiwavelength catalog (Guo+, 2013)J/ApJS/206/8 : COSMOS/UltraVISTA Ks-selected catalogs v4.1 (Muzzin+, 2013)J/ApJS/214/24 : 3D-HST+CANDELS catalog (Skelton+, 2014)J/ApJ/801/97 : GOODS-S & UDS stellar masses from CANDELS (Santini+, 2015)J/ApJ/830/51 : FourStar galaxy evolution (ZFOURGE) (Straatman+, 2016)J/A+A/608/A2 : MUSE Hubble Ultra Deep Field Survey. II. (Inami+, 2017)J/ApJ/844/171 : Ly{alpha} profile in 43 Green Pea galaxies (Yang+, 2017)J/ApJS/228/7 : Multi-wavelength data in CANDELS COSMOS (Nayyeri+, 2017)J/ApJS/229/32 : CANDELS: multiwavelength cat. in the EGS (Stefanon+, 2017)J/MNRAS/478/4293 : 0.1<z<0.8 gal. gas-phase metallicity grad. (Carton+, 2018)J/A+A/624/A141 : MUSE-Wide Survey DR1 catalog (Urrutia+, 2019)J/ApJ/888/79 : Emission-line galaxies from the FIGS survey (Pharo+, 2020)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/261/12https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/261/12http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/261/12https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/261/12https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/261/12http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/261/12GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/261/12/catalog (Redshift (Table 3) and emission line flux (Table 4) catalog)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/261/12/catalog?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/261/12/catalog?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/261/12/catalog?GETtext/xml+votable180.050000true150.00152.48450.0055555555555555566/11252 11425 27256 27258 359351.1796835550914393e-19 3.9057996558789745e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/261/12?format=asciidefaultJ/ApJS/261/12/catalogRedshift (Table 3) and emission line flux (Table 4) catalogSimbadNameSimbad column added by the CDSmeta.idcharnullablezH7[0.075/1.52]? Redshift from HALO7D spectrumsrc.redshift;pos.heliocentricfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordinte_HbF[0.4/257]? Uncertainty in HbF1e-19mW.m**-2stat.errorfloatnullableSNHbF[1/38]? Signal-to-Noise of HbFstat.snrfloatnullableHbEW[0.1/1327]? H{beta} equivalent width in {AA}0.1nmspect.line.eqWidthfloatnullableO3-59F[0/3328]? The [OIII]4959{AA} line flux (6)1e-19mW.m**-2phot.flux;spect.linefloatnullablee_O3-59F[0/250]? Uncertainty in O3-59F1e-19mW.m**-2stat.errorfloatnullableq_zH7[0/3] Quality flag on zH7 (3=secure) (1)meta.code.qualintzELC[0/7] Emission line count for the redshift catalogmeta.numberintALC[0/1] Absorption line countmeta.numberintFieldAbbreviated CANDELS field identifiermeta.id;obs.fieldcharHALO7DHALO7D survey identifiermeta.idcharCANDELSCANDELS catalog identifiermeta.idcharOtherOther identifier (or "-99.0")meta.idcharRAJ2000[52.9/215.5] Right Ascension (J2000)degpos.eq.ra;meta.mainDEJ2000[-28/62.4] Declination (J2000)degpos.eq.dec;meta.mainzph[0/6.25]? Photometric derived redshift (3)src.redshiftfloatnullablezsp[0.004/3.75]? Spectroscopic derived redshift (3)src.redshiftdoublenullablelogM[0/13.15]? Log stellar mass from SED fittinglog(solMass)phys.massfloatnullableSFR[-26.2/3.3]? Star formation rate from SED fittingsolMass/yrphys.SFRdoublenullableExp[0.7/156.5] Total HALO7D exposure timehtime.duration;obs.exposurefloatF606Wmag[14.7/28.1]? HST F606W band apparent AB magnitudemagphot.mag;em.opt.RfloatnullableF814Wmag[14.2/28]? HST F814W band apparent AB magnitudemagphot.mag;em.opt.IfloatnullableF160Wmag[14.1/26.8]? HST/WFC3 F160W (H-band) apparent AB magnitudemagphot.mag;em.IR.HfloatnullableE(B-V)[-49.5/0.76]? The (B-V) color excess (4)magphot.color.excessfloatnullableU-V[-0.9/3]? The (U-V) color index (4)phot.color;em.opt.U;em.opt.VfloatnullableV-J[-3/3.4]? The (V-J) color index (4)phot.color;em.opt.V;em.IR.JfloatnullableELC[0/7] Emission line count for the emission line flux catalog (5)meta.numberintLinesDetected line identifiers for the emission line flux catalogmeta.id;spect.linecharO2F[0/9946]? Summed [OII]3727,3729{AA} line flux (6)1e-19mW.m**-2phot.flux;spect.linefloatnullablee_O2F[0/1237]? Uncertainty in O2F1e-19mW.m**-2stat.errorfloatnullableSNO2F[1/52]? Signal-to-Noise of O2Fstat.snrfloatnullablef_SNO2F[i] i=nan or inf valuemeta.codecharO2EW[0.3/2644]? The [OII]3727,3729{AA} equivalent width in {AA}0.1nmspect.line.eqWidthfloatnullablef_O2EW[i] i=nan or inf valuemeta.codecharHdF[0.5/5249]? H{delta} line flux (6)1e-19mW.m**-2phot.flux;spect.linefloatnullablee_HdF[0.5/1307]? Uncertainty in HdF1e-19mW.m**-2stat.errorfloatnullableSNHdF[1/28]? Signal-to-Noise of HdFstat.snrfloatnullableHdEW[0.1/696]? H{delta} equivalent width in {AA}0.1nmspect.line.eqWidthfloatnullableHgF[1.4/1517]? H{gamma} line flux (6)1e-19mW.m**-2phot.flux;spect.linefloatnullablee_HgF[0.2/160]? Uncertainty in HgF1e-19mW.m**-2stat.errorfloatnullableSNHgF[1/37]? Signal-to-Noise of HgFstat.snrfloatnullableHgEW[0.1/1063]? H{gamma} equivalent width in {AA}0.1nmspect.line.eqWidthfloatnullableHbF[1.8/4447]? H{beta} line flux (6)1e-19mW.m**-2phot.flux;spect.linefloatnullableSNO3-59F[0/33]? Signal-to-Noise of O3-59Fstat.snrfloatnullablef_SNO3-59F[i] i=nan or inf valuemeta.codecharO3-59EW[0.04/4961]? The [OIII]5007{AA} equivalent width in {AA}0.1nmspect.line.eqWidthfloatnullablef_O3-59EW[i] i=nan or inf valuemeta.codecharO3-07F[0/9984]? The [OIII]5007{AA} line flux (6)1e-19mW.m**-2phot.flux;spect.linefloatnullablee_O3-07F[0/748]? Uncertainty in O3-07F1e-19mW.m**-2stat.errorfloatnullableSNO3-07F[1.2/33]? Signal-to-Noise of O3-07Fstat.snrfloatnullablef_SNO3-07F[i] i=nan or inf valuemeta.codecharO3-07EW[0.1/14883]? The [OIII]5007{AA} equivalent width in {AA}0.1nmspect.line.eqWidthdoublenullablef_O3-07EW[i] i=nan or inf valuemeta.codecharHaF[13/8420]? H{alpha} line flux (6)1e-19mW.m**-2phot.flux;spect.linefloatnullablee_HaF[4/490]? Uncertainty in HaF1e-19mW.m**-2stat.errorfloatnullableSNHaF[1/25]? Signal-to-Noise of HaFstat.snrfloatnullableHaEW[0.46/271]? H{alpha} equivalent width in {AA}0.1nmspect.line.eqWidthfloatnullableCatDisplay data from Muzzin+, 2013, J/ApJS/206/8 ; Nayyeri+, 2017, J/ApJS/228/7 ; Stefanon+, 2017, J/ApJS/229/32 ; Barro+, 2011, J/ApJS/193/13 ; Guo+, 2013, J/ApJS/207/24 and GOODS (II/318) within 0.5"meta.ref.urlintnullableIDIdentifiermeta.id;meta.maincharzLinesDetected line identifiers for the redsfhit catalogmeta.id;spect.linechar