J/ApJS/264/19ivo://CDS.VizieR/J/ApJS/264/19doi:10.26093/cds/vizier.22640019CDSHyun M.Im M.Smail I.R.Cotton W.D.Birkin J.E.Kikuta S.Shim H.,Willmer C.N.A.Condon J.J.Windhorst R.A.Cohen S.H.Jansen R.A.,Ly C.Matsuda Y.Fazio G.G.Swinbank A.M.Yan H.2023-08-25T12:16:20Z2023-04-19T10:06:46ZCDS support team

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

cds-question@unistra.frradio-galaxiesmillimeter-astronomysubmillimeter-astronomysurveysredshiftedinfrared-photometryinterstellar-reddeningvisible-astronomyspectroscopyThe James Webb Space Telescope Time-Domain Field (JWST-TDF) is an ~14' diameter field near the North Ecliptic Pole that will be targeted by one of the JWST Guaranteed Time Observations programs. Here, we describe our James Clerk Maxwell Telescope SCUBA-2 850um imaging of the JWST-TDF and present the submillimeter source catalog and properties. We also present a catalog of radio sources from Karl J. Jansky Very Large Array 3GHz observations of the field. These observations were obtained to aid JWST's study of dust-obscured galaxies that contribute significantly to cosmic star formation at high redshifts. Our deep 850um map covers the JWST-TDF at a noise level of {sigma}_850um_=1.0mJy/beam, detecting 83/31 sources in the main/supplementary signal-to-noise ratio (S/N>4 / S/N=3.5-4) sample, respectively. The 3GHz observations cover a 24' diameter field with a 1{sigma} noise of 1uJy/beam at a 0.7" FWHM. We identified eighty-five 3GHz counterparts to sixty-six 850um sources and then matched these with multiwavelength data from the optical to the mid-infrared wave bands. We performed spectral energy distribution fitting for 61 submillimeter galaxies (SMGs) matched with optical/near-infrared data, and found that SMGs at S/N>4 have a median value of z_phot_=2.22+/-0.12, star formation rates of 300+/-40M_{sun}_/yr (Chabrier initial mass function), and typical cold dust masses of 5.9+/-0.7x10^8^M_{sun}_, in line with bright SMGs from other surveys. The large cold dust masses indicate correspondingly large cool gas masses, which we suggest are a key factor necessary to drive the high star formation rates seen in this population.2023ApJS..264...19Hhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/264/19CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/jcmt : Jame Clerk Maxwell Telescope Science Archive (CADC, 2003)II/311 : WISE All-Sky Data Release (Cutri+ 2012)II/328 : AllWISE Data Release (Cutri+ 2013)J/ApJ/622/772 : Redshift survey of submillimeter galaxies (Chapman+, 2005)J/MNRAS/372/1621 : SCUBA Half-Degree Extragalactic Survey. II (Coppin+, 2006)J/MNRAS/380/199 : SCUBA Half-Degree Extragalactic Survey. III (Ivison+, 2007)J/MNRAS/385/2225 : AzTEC millimetre survey of COSMOS field (Scott+, 2008)J/ApJ/707/1201 : LABOCA ECDFS Submillimeter Survey (LESS) (Weiss+, 2009)J/A+A/532/A90 : PACS Evolutionary Probe (PEP-DR1) catalogs (Lutz+, 2011)J/MNRAS/436/1919 : SCUBA observations of COSMOS galaxies (Casey+, 2013)J/ApJ/788/125 : ALMA survey of ECDFS submillimeter galaxies (Simpson+, 2014)J/ApJ/804/34 : Luminous AGNs and early-type SDSS galaxies (Hong+, 2015)J/ApJ/806/110 : ALESS survey: SMGs in the ECDF-S data (da Cunha+, 2015)J/ApJ/820/83 : ALMA galaxies in the COSMOS survey field (Scoville+, 2016)J/MNRAS/464/3369 : SCUBA-2 EGS deep field (Zavala+, 2017)J/MNRAS/465/1789 : SCUBA-2 Cosmology Legacy Survey (Geach+, 2017)J/ApJ/837/139 : SUPER GOODS. I. Ultradeep SCUBA-2 survey (Cowie+, 2017)J/ApJ/856/67 : VLA 3GHz radio sources in the Lockman Hole (Cotton+, 2018)J/ApJ/865/106 : SUPER GOODS. III. SCUBA-2 sources with ALMA (Cowie+, 2018)J/ApJ/880/43 : S2COSMOS: bright SCUBA-2 submm sources (Simpson+, 2019)J/MNRAS/487/4648 : ALMA survey of the SCUBA-2 UKIDSS/UDS field (Stach+, 2019)J/ApJ/886/48 : Rad, opt/NIR counterparts of S2COSMOS submm gal. (An+, 2019)J/A+A/644/A144 : Dusty star-forming galaxies properties (Donevski+, 2020)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/264/19https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/264/19http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/264/19https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/264/19https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/264/19http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/264/19GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/264/19/table3 (*VLA 3GHz source catalog)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/264/19/table3?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/264/19/table3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/264/19/table3?GETtext/xml+votable180.050000true260.32761166765.7939127780.005555555555555556Cone search capability for table J/ApJS/264/19/table4 (*Full version of James Webb Space Telescope Time-Domain Field (JWST-TDF) SCUBA-2 850um source catalog)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/264/19/table4?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/264/19/table4?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/264/19/table4?GETtext/xml+votable180.050000true260.4070843465.799071880.0055555555555555566/116081.987820871092403e-24 4.963257411639215e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/264/19?format=asciiOpticalInfraredMillimeterRadiodefaultJ/ApJS/264/19/table3*VLA 3GHz source catalogrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/756] Running sequence number (VLA_ID)meta.id;meta.maininte_RA[0/0.0376] RA uncertainty (dRA)arcsecstat.error;pos.eq.radoubleRAJ2000Hour of right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Degree of declination (J2000)pos.eq.dec;meta.maine_DE[0/0.249] DE uncertainty (dDec)arcsecstat.error;pos.eq.decfloatS3GHz[4.7/210000] VLA 3GHz flux density, corrected for the primary beamuJyphot.flux.density;em.radio.1500-3000MHzdoublee_S3GHz[0/283.1] S3GHz uncertainty (dS3GHz)uJystat.errorfloatf_SizeUpper limit flag on Size or LAS (1)meta.codecharSize[0.1/36.5] Deconvolved angular size or largest angular size (Major)arcsecphys.angSizefloate_Size[0.03/]? Size uncertainty (dMajor)arcsecstat.error;phys.angSizefloatnullablel_MinorUpper limit flag on Minormeta.code.errorcharMinor[0.24/1.58]? Minor axisarcsecphys.angSize;srcfloatnullablee_Minor[0.03/0.23]? Minor uncertainty (dMinor)arcsecstat.errorfloatnullablePA[-89/90]? Position angledegpos.posAngintnullablee_PA[1/90]? PA uncertainty (dPA)degstat.errorintnullableF850Display the JWST-TDF SCUBA-2 850um data if any (link to Table 4)meta.ref.urlintnullableJ/ApJS/264/19/table4*Full version of James Webb Space Telescope Time-Domain Field (JWST-TDF) SCUBA-2 850um source catalogB_Mstar[10/13]? Mstar upper bound (Mstar_u)log(solMass)phys.mass;stat.maxfloatnullableb_Ldust[10.5/13.5]? Ldust lower bound (L_dust_l)log(solLum)phys.luminosity;stat.minfloatnullableLdust[10.5/13.5]? Log of dust luminosity (L_dust)log(solLum)phys.luminosityfloatnullableB_Ldust[11/13.6]? Ldust upper bound (L_dust_u)log(solLum)phys.luminosity;stat.maxfloatnullableb_Tdust[27.2/77.8]? Tdust lower bound (Tdust_l)Kphys.temperature;stat.minfloatnullableTdust[29.7/78]? Kinetic dust temperature (Tdust)Kphys.temperaturefloatnullableB_Tdust[36.3/77.8]? Tdust upper bound (Tdust_u)Kphys.temperature;stat.maxfloatnullableb_SFR[0.16/3.11]? SFR lower bound (SFR_l)log(solMass.yr**-1)phys.SFR;stat.minfloatnullableSFR[0.17/3.5]? Log of star formation rate (SFR)log(solMass.yr**-1)phys.SFRfloatnullableB_SFR[0.6/3.7]? SFR upper bound (SFR_u)log(solMass.yr**-1)phys.SFR;stat.maxfloatnullableb_Mdust[7/9.4]? Mdust lower bound (Mdust_l)log(solMass)phys.mass;stat.minfloatnullableNi[8.8e-7/0.0006]? Radio source number density S_3GHz_>Simeta.numberdoublenullablePc[0.10628612]? Pc={pi}r_s_^2^N_T_, Equation (8) (always "0.10628612")stat.fit.goodnessdoublenullablePst[4e-6/0.03]? P^*^={pi}r_i_^2^N_i_, Equation (9) (Pstar)stat.fit.goodnessdoublenullablep[4.5e-5/0.07]? Corrected Poissonian probability, Equation (6) (p=1-exp(-E))stat.probabilitydoublenullableB_Mdust[7.7/9.8]? Mdust upper bound (Mdust_u)log(solMass)phys.mass;stat.maxfloatnullableb_Age[7/9.3]? Age lower bound (Age_l)log(yr)time.age;stat.minfloatnullableAge[7/9.3]? Log of Age (Age)log(yr)time.agefloatnullableNrad[1/3]? Number of radio counterparts (n_radio_counterpart)meta.numberintnullableRank[1/3]? Rank of the radio-matched object based on the separated distance (closest_rank)meta.numberintnullableF850um[2.8/19.7] Peak JCMT 850um flux (JCMT_FLUX_PEAK)mJyphot.flux.density;em.mm.200-400GHzdoublee_F850um[0.7/1.5] F850um rms uncertainty (JCMT_RMS_PEAK)mJystat.errordoubleFMod[2.3/19.7] Model JCMT 850um flux (JCMT_FLUX_MODEL)mJyphot.flux.density;em.mm.200-400GHz;meta.modelleddoublee_FMod[0.7/1.5] FMod rms uncertainty (JCMT_RMS_MODEL)mJystat.errordoubleSN850[3.5/20.2] JCMT 850um S/N (JCMT_SNR)stat.snrdoubleBlend[0/1]? 1=blend (JCMT_BLEND)meta.codeintnullableF850d[1.9/19] Deboosted JCMT 850um flux (JCMT_FLUX_DEBOOST)mJyphot.flux.density;em.mm.200-400GHzfloate_F850d[0.5/2.5] Lower uncertainty in F850d (JCMT_FLUX_DEBOOST_ERRLO)mJystat.errorfloatE_F850d[0.7/2.2] Upper uncertainty in F850d (JCMT_FLUX_DEBOOST_ERRHI)mJystat.error;stat.maxfloaterlF850d[0.9/2.7] Lower total uncertainty in F850d (JCMT_TOTAL_ERRLO)mJystat.error;stat.minfloateruF850d[1.1/2.7] Upper total uncertainty in F850d (JCMT_TOTAL_ERRHI)mJystat.error;stat.maxfloatRAJ2000[260.3/261.1] Peak flux right ascension (J2000) (JCMT_RA_PEAK_DEG_FIN)degpos.eq.ra;meta.mainDEJ2000[65.6/66] Peak flux declination (J2000) (JCMT_DEC_PEAK_DEG_FIN)degpos.eq.dec;meta.mainRAMdeg[260.3/261.1] Peak model flux right ascension (JCMT_RA_MODEL_DEG_FIN)degpos.eq.raDEMdeg[65.6/66] Peak model flux declination (JCMT_DEC_MODEL_DEG_FIN)degpos.eq.decVLAID[9/666]? Identifier from VLA catalog (Table 3) (ID_VLA)meta.id.crossintnullableRAVdeg[260.3/261.1]? VLA right ascension in decimal degrees (J2000) (RA_VLA)degpos.eq.ranullableDEVdeg[65.6/66]? VLA Declination in decimal degrees (J2000) (DEC_VLA)degpos.eq.decnullableS3GHz[5.4/210000]? 3GHz radio flux (radio_flux)uJyphot.flux.density;em.radio.1500-3000MHzdoublenullablee_S3GHz[0/13]? S3GHz uncertainty (dS3GHz)uJystat.errordoublenullableSep[0.1/7.8]? Angular separation between VLA and JCMT (angular_distance)arcsecpos.angDistancefloatnullableSED[1/3]? SED group (sed_group) (1)meta.codeintnullablegmagAp[17.6/28.1]? g-band aperture magnitude from Subaru/HSC (GMAG_APER_300)magphot.mag;em.opt.Bfloatnullablee_gmagAp[0.01/14]? GmagAp uncertainty (GMAGERR_APER_300)magstat.errordoublenullableimagAp[17.2/26]? i-band aperture magnitude from Subaru/HSC (IMAG_APER_300)magphot.mag;em.opt.Ifloatnullablee_imagAp[0.01/2.3]? ImagAp uncertainty (IMAGERR_APER_300)magstat.errordoublenullablezmagAp[17/26.6]? z-band aperture magnitude from Subaru/HSC (ZMAG_APER_300)magphot.mag;em.opt.Ifloatnullablee_zmagAp[0.01/4.5]? zmagAp uncertainty (ZMAGERR_APER_300)magstat.errordoublenullableYmagAp[17.2/26.1]? Y-band aperture magnitude from MMT/MMIRS (YMAG_APER_3)magphot.mag;em.IR.Jfloatnullablee_YmagAp[0.001/1.2]? YmagAp uncertainty (YMAGERR_APER_3)magstat.errordoublenullableJmagAp[16/23.1]? J-band aperture magnitude from MMT/MMIRS (JMAG_APER_3)magphot.mag;em.IR.Jfloatnullablee_JmagAp[0.0008/0.2]? JmagAp uncertainty (JMAGERR_APER_3)magstat.errordoublenullableHmagAp[15.3/22.1]? H-band aperture magnitude from MMT/MMIRS (HMAG_APER_3)magphot.mag;em.IR.Hfloatnullablee_HmagAp[0.0004/0.02]? HmagAp uncertainty (HMAGERR_APER_3)magstat.errordoublenullableKmagAp[15.3/22.3]? K-band aperture magnitude from MMT/MMIRS (KMAG_APER_3)magphot.mag;em.IR.Kdoublenullablee_KmagAp[0.0008/0.5]? KmagAp uncertainty (KMAGERR_APER_3)magstat.errordoublenullablee_W1mag[0.003/0.05]? Uncertainty in W1mag (dw1)magstat.error;phot.magfloatnullableW2mag[22/23.7]? WISE W2 (4.6um) band AB magnitude (w2_ab)magphot.mag;em.IR.4-8umfloatnullablee_W2mag[0.004/0.07]? Uncertainty in W2mag (dw2)magstat.error;phot.magfloatnullablel_W3magUpper limit flag on W3magmeta.code.errorcharW3mag[15.6/19]? WISE W3 (12um) band AB magnitude (w3_ab)magphot.flux.density;em.IR.8-15umfloatnullablee_W3mag[0.03/0.6]? Uncertainty on the W3mag (w3msigmpro)magstat.error;phot.magfloatnullablel_W4magUpper limit flag on W4magmeta.code.errorcharW4mag[14.6/16.8]? WISE W4 (22um) band AB magnitude (w4_ab)magphot.flux.density;em.IR.15-30umfloatnullablee_W4mag[0.1/0.5]? Uncertainty on the W4mag (w4msigmpro)magstat.error;phot.magfloatnullablel_amajUpper limit flag on amajmeta.code.errorcharamaj[0.1/2.1]? Ellipse-fit major axis (Major)arcsecphys.angSizefloatnullablee_amaj[0.03/0.4]? amaj uncertainty (dMajor)arcsecstat.errorfloatnullablel_bminUpper limit flag on bminmeta.code.errorcharbmin[0.24/0.98]? Ellipse-fit minor axis (Minor)arcsecphys.angSize;srcfloatnullablee_bmin[0.05/0.2]? bmin uncertainty (dMinor)arcsecstat.errorfloatnullablePA[-70/90]? Position angle (PA)degpos.posAngintnullablee_PA[2/42]? PA uncertainty (dPA)degstat.errorintnullablechi2[0/11]? {chi}^2^ of the SED fitting result (chi)stat.fitdoublenullableb_Mstar[9.7/12.5]? Mstar lower bound (Mstar_l)log(solMass)phys.mass;stat.minfloatnullableMstar[9.8/12.8]? Log of stellar mass (Mstar)log(solMass)phys.massfloatnullableMdust[7.5/9.6]? Log of dust mass (Mdust)log(solMass)phys.massfloatnullableB_Age[7.3/9.5]? Age upper bound (Age_u)log(yr)time.age;stat.maxfloatnullableb_Av[0.2/7.3]? Av lower bound (AV_l)magphot.mag;stat.minfloatnullableW1mag[21.8/23.5]? WISE W1 (3.4um) band AB magnitude (w1_ab)magphot.mag;em.IR.3-4umfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeq[1/133]? Running sequence number (index)meta.idintnullableJCMTInd[1/114] JCMT index (JCMT_index)meta.idintS2TDFIAU position-based name, (JHHMMSS+DDMMSS) (JCMT_ID)meta.id;meta.maincharANameShort name: S2TDF.0{JCMTInd} (JCMT_SHORT_ID)meta.idcharm_ANameIdentifier with VLA multiplicity index, {AName}.[0-2] (ID)meta.code.multipcharVLA[0/1] True = VLA match (Got_VLA_ID)meta.codeintSNR[0/1] True = high SNR (High_SNR)meta.codeintnVLA[0/1] True = no VLA match (NOT_Got_VLA_ID)meta.codeintClose[0/1] True = closest matched object (Closest_ID)meta.codeintMult[0/1] True = multiple VLA matches (Multiple_IDs)meta.codeintNS[1/624]? Radio source number density S_3GHz_>10uJy (N(S>S))meta.numberintnullableAv[0.2/9.6]? V-band reddeningmagphys.absorptionfloatnullableB_Av[0.2/12]? Av upper bound (AV_u)magphot.mag;stat.maxfloatnullableb_tau[0.4/12.7]? tau lower bound (tau_l)Gyrphys.SFR;stat.minfloatnullabletau[0.4/16.1]? Star formation timescale parameter (tau)Gyrphys.SFRfloatnullableB_tau[0.4/18.8]? tau upper bound (tau_u)Gyrphys.SFR;stat.maxfloatnullableb_sSFR[-10.5/-7.9]? sSFR lower bound (sSFR_l)log(yr**-1)phys.SFR;stat.minfloatnullablesSFR[-10.4/-7.9]? Log of specific SFR (sSFR)log(yr**-1)phys.SFRfloatnullableB_sSFR[-10.1/-7.9]? sSFR upper bound (sSFR_u)log(yr**-1)phys.SFR;stat.maxfloatnullableb_zmed[0.2/3.5]? zmed lower bound (z_lower)meta.notefloatnullablezmed[0.2/3.8]? Median photometric redshift (z_med)src.redshift.photfloatnullableB_zmed[0.3/7.6]? zmed upper bound (z_upper)meta.notefloatnullableb_E(B-V)[0.03/0.7]? E(B-V) lower bound (eb_l)magphot.color;stat.minfloatnullableE(B-V)[0.1/1]? Color excess (eb)magphot.color.excessfloatnullableB_E(B-V)[0.1/1]? E(B-V) upper bound (eb_u)magphot.color;stat.maxfloatnullableNotesNotesmeta.notecharWISEDisplay the WISE (II/311) and AllWISE (II/328) data within 7" if W1mag is filledmeta.ref.urlchar