J/AJ/151/120ivo://CDS.VizieR/J/AJ/151/120doi:10.26093/cds/vizier.51510120CDSWesthues C.Haas M.Barthel P.Wilkes B.J.Willner S.P.,Kuraszkiewicz J.Podigachoski P.Leipski C.Meisenheimer K.,Siebenmorgen R.Chini R.2021-12-16T13:37:06Z2018-04-11T12:15:26ZCDS support team

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

cds-question@unistra.frradio-galaxiesquasarsactive-galactic-nucleispectroscopyinfrared-photometryspectral-energy-distributionchemical-abundancesstellar-agesstellar-massesUsing the Herschel Space Observatory we have observed a representative sample of 87 powerful 3CR sources at redshift z<1. The far-infrared (FIR, 70-500 {mu}m) photometry is combined with mid-infrared (MIR) photometry from the Wide-Field Infrared Survey Explorer and cataloged data to analyze the complete spectral energy distributions (SEDs) of each object from optical to radio wavelength. To disentangle the contributions of different components, the SEDs are fitted with a set of templates to derive the luminosities of host galaxy starlight, dust torus emission powered by active galactic nuclei (AGNs), and cool dust heated by stars. The level of emission from relativistic jets is also estimated to isolate the thermal host galaxy contribution. The new data are in line with the orientation-based unification of high-excitation radio-loud AGN, in that the dust torus becomes optically thin longwards of 30 {mu}m. The low-excitation radio galaxies and the MIR-weak sources represent an MIR- and FIR-faint AGN population that is different from the high-excitation MIR-bright objects; it remains an open question whether they are at a later evolutionary state or an intrinsically different population. The derived luminosities for host starlight and dust heated by star formation are converted to stellar masses and star-formation rates (SFR). The host-normalized SFR of the bulk of the 3CR sources is low when compared to other galaxy populations at the same epoch. Estimates of the dust mass yield a 1-100 times lower dust/stellar mass ratio than for the Milky Way, which indicates that these 3CR hosts have very low levels of interstellar matter and explains the low level of star formation. Less than 10% of the 3CR sources show levels of star formation above those of the main sequence of star-forming galaxies.2016AJ....151..120Whttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/151/120CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVIII/1 : The 3C and 3CR Catalogues (Edge+ 1959-1962)VI/139 : Herschel Observation Log (Herschel Science Centre, 2013)J/MNRAS/204/151 : Bright radio sources at 178 MHz (3CRR) (Laing+ 1983)J/PASP/97/932 : 3CR Source Identifications (Spinrad+, 1985)J/A+A/575/A80 : FIR photometry of 3CR galaxies (Podigachoski+, 2015)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/151/120https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/151/120http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/151/120https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/151/120https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/151/120http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/151/120GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/AJ/151/120/table1 (3CR Sources 0.5<z<1 Observed with Herschel)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/151/120/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/151/120/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/151/120/table1?GETtext/xml+votable180.050000true4.12958379.2805560.005555555555555556Cone search capability for table J/AJ/151/120/table2 (3CR Sources z<0.5 Observed with Herschel)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/AJ/151/120/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/AJ/151/120/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/AJ/151/120/table2?GETtext/xml+votable180.050000true10.78833352.060.0055555555555555566/245 1129 1263 1521 2052 2125 2227 2245 2866 2949 2951 3803 4014 4285 4352 4376 4835 5027 5284 5311 5439 5806 5817 6618 6889 7061 7508 7888 7925 8017 8043 8152 8528 8555 8675 8809 8989 9009 9230 9252 9273 9655 9992 10004 10217 10432 10839 10877 11073 11259 11365 11512 11551 11667 11874 12010 12047 12335 12796 13120 13455 13707 13855 14858 15045 15064 15067 15909 16189 16301 18365 18387 18895 19325 22452 22505 23323 23469 23476 24023 24116 26292 28063 28279 28574 320593.2031150387835462e-22 3.243176138527326e-21https://cdsarc.cds.unistra.fr/viz-bin/moc/J/AJ/151/120?format=asciiInfraredRadiodefaultJ/AJ/151/120/table13CR Sources 0.5<z<1 Observed with HerschelSimbadNameSimbad column added by the CDSmeta.idcharnullableTypeType of galaxy (2)src.classcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint3C[006.1/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloatRAJ2000Hour of Right Ascension (J2000)pos.eq.ra;meta.mainDEJ2000Degree of Declination (J2000)pos.eq.dec;meta.mainn_DEJ2000[c] Note on DEs (1)meta.notecharz[0.0169/0.996] Redshiftsrc.redshiftfloatDL[66/6426] Luminosity distanceMpcpos.distanceintn_Type[b,c d] Note(s) on Type (1)meta.notecharPID[1/6] Proposal identifier (3)meta.codeintPObsID1? Herschel/PACS first ObsIDmeta.id;obsnullablePObsID2? Herschel/PACS second ObsIDmeta.id;obsnullablePObsID3? Herschel/PACS third ObsIDmeta.id;obsnullablePObsID4? Herschel/PACS fourth ObsIDmeta.id;obsnullableSPObsID[1342229105/1342268340]? Herschel/SPIRE ObsIDmeta.id;obslongnullableJ/AJ/151/120/table23CR Sources z<0.5 Observed with HerschelSimbadNameSimbad column added by the CDSmeta.idcharnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint3C[006.1/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloatRAJ2000Hour of Right Ascension (J2000)pos.eq.ra;meta.mainDEJ2000Degree of Declination (J2000)pos.eq.dec;meta.mainn_DEJ2000[c] Note on DEs (1)meta.notecharz[0.0169/0.996] Redshiftsrc.redshiftfloatDL[66/6426] Luminosity distanceMpcpos.distanceintTypeType of galaxy (2)src.classcharn_Type[b,c d] Note(s) on Type (1)meta.notecharPID[1/6] Proposal identifier (3)meta.codeintPObsID1? Herschel/PACS first ObsIDmeta.id;obsnullablePObsID2? Herschel/PACS second ObsIDmeta.id;obsnullablePObsID3? Herschel/PACS third ObsIDmeta.id;obsnullablePObsID4? Herschel/PACS fourth ObsIDmeta.id;obsnullableSPObsID[1342229105/1342268340]? Herschel/SPIRE ObsIDmeta.id;obslongnullableJ/AJ/151/120/table43CR Sources 0.5<z<1 PACS and SPIRE Flux Densities3C[006.1/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintFig[1/15] Figure number in the papermeta.idintl_F70[<] Limit flag on F70meta.code.errorcharF70[6/783]? Herschel/PACS 70 {mu}m flux densitymJyphot.flux.density;em.IR.30-60umintnullablee_F70[2/8]? 1{sigma} uncertainty in F70mJystat.errorintnullablel_F100[<] Limit flag on F100meta.code.errorcharF100[6/867]? Herschel/PACS 100 {mu}m flux densitymJyphot.flux.density;em.IR.60-100umintnullablee_F100[1/6]? 1{sigma} uncertainty in F100mJystat.errorintnullablel_F160[<] Limit flag on F160meta.code.errorcharF160[13/1347]? Herschel/PACS 160 {mu}m flux densitymJyphot.flux.density;em.mm.1500-3000GHzintnullablee_F160[3/24]? 1{sigma} uncertainty in F160mJystat.errorintnullablel_F250[<] Limit flag on F250meta.code.errorcharF250[22/955]? Herschel/SPIRE 250 {mu}m flux densitymJyphot.flux.density;em.mm.750-1500GHzintnullablee_F250[8/27]? 1{sigma} uncertainty in F250mJystat.errorintnullablel_F350[<] Limit flag on F350meta.code.errorcharF350[20/741]? Herschel/SPIRE 350 {mu}m flux densitymJyphot.flux.density;em.mm.750-1500GHzintnullablee_F350[8/26]? 1{sigma} uncertainty in F350mJystat.errorintnullablel_F500[<] Limit flag on F500meta.code.errorcharF500[23/1062]? Herschel/SPIRE 500{mu}m flux densitymJyphot.flux.density;em.mm.400-750GHzintnullablee_F500[7/31]? 1{sigma} uncertainty in F500mJystat.errorintnullableJ/AJ/151/120/table53CR Sources z<0.5 PACS and SPIRE Flux DensitiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint3C[006.1/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloatFig[1/15] Figure number in the papermeta.idintl_F70[<] Limit flag on F70meta.code.errorcharF70[6/783]? Herschel/PACS 70 {mu}m flux densitymJyphot.flux.density;em.IR.30-60umintnullablee_F70[2/8]? 1{sigma} uncertainty in F70mJystat.errorintnullablel_F100[<] Limit flag on F100meta.code.errorcharF100[6/867]? Herschel/PACS 100 {mu}m flux densitymJyphot.flux.density;em.IR.60-100umintnullablee_F100[1/6]? 1{sigma} uncertainty in F100mJystat.errorintnullablel_F160[<] Limit flag on F160meta.code.errorcharF160[13/1347]? Herschel/PACS 160 {mu}m flux densitymJyphot.flux.density;em.mm.1500-3000GHzintnullablee_F160[3/24]? 1{sigma} uncertainty in F160mJystat.errorintnullablel_F250[<] Limit flag on F250meta.code.errorcharF250[22/955]? Herschel/SPIRE 250 {mu}m flux densitymJyphot.flux.density;em.mm.750-1500GHzintnullablee_F250[8/27]? 1{sigma} uncertainty in F250mJystat.errorintnullablel_F350[<] Limit flag on F350meta.code.errorcharF350[20/741]? Herschel/SPIRE 350 {mu}m flux densitymJyphot.flux.density;em.mm.750-1500GHzintnullablee_F350[8/26]? 1{sigma} uncertainty in F350mJystat.errorintnullablel_F500[<] Limit flag on F500meta.code.errorcharF500[23/1062]? Herschel/SPIRE 500{mu}m flux densitymJyphot.flux.density;em.mm.400-750GHzintnullablee_F500[7/31]? 1{sigma} uncertainty in F500mJystat.errorintnullableJ/AJ/151/120/table6Median Spectral Templates for Different Galaxy Types Separated for Low- (z<0.5) and Medium-redshift (0.5<z<1)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlog(lrest)[-0.4/6.6] Log of rest wavelength {lambda}_Rest_log(um)em.wlfloatlog(nuLnu)Hl[8.7/11.1] Log of rest frame luminosity {nu}L_{nu}_ for high-excitation radio low-z galaxy typelog(solLum)phys.luminosityfloate_log(nuLnu)Hl[0.1/1] Uncertainty in log(nuLnu)Hllog(solLum)stat.errorfloatlog(nuLnu)Hm[10/11.5] Log of rest frame luminosity {nu}L_{nu}_ for high-excitation radio medium-z galaxy typelog(solLum)phys.luminosityfloate_log(nuLnu)Hm[0.1/0.7] Uncertainty in log(nuLnu)Hmlog(solLum)stat.errorfloatlog(nuLnu)L[8.7/11.2]? Log of rest frame luminosity {nu}L_{nu}_ for low-excitation radio galaxy typelog(solLum)phys.luminosityfloatnullablee_log(nuLnu)L[0.1/1.3]? Uncertainty in log(nuLnu)Llog(solLum)stat.errorfloatnullablelog(nuLnu)B[9.1/11.5]? Log of rest frame luminosity {nu}L_{nu}_ for broad-line radio galaxy typelog(solLum)phys.luminosityfloatnullablee_log(nuLnu)B[0.1/0.9]? Uncertainty in log(nuLnu)Blog(solLum)stat.errorfloatnullablelog(nuLnu)Fl[8.4/11]? Log of rest frame luminosity {nu}L_{nu}_ for flat-spectrum low-z quasar typelog(solLum)phys.luminosityfloatnullablee_log(nuLnu)Fl[0.3/0.8]? Uncertainty in log(nuLnu)Fllog(solLum)stat.errorfloatnullablelog(nuLnu)Fm[10.2/12.1]? Log of rest frame luminosity {nu}L_{nu}_ for flat-spectrum medium-z quasar typelog(solLum)phys.luminosityfloatnullablee_log(nuLnu)Fm[0.2/0.3]? Uncertainty in log(nuLnu)Fmlog(solLum)stat.errorfloatnullablelog(nuLnu)Sl[10.2/12.2]? Log of rest frame luminosity {nu}L_{nu}_ for steep-spectrum low-z quasar typelog(solLum)phys.luminosityfloatnullablee_log(nuLnu)Sl[0.2/1.6]? Uncertainty in log(nuLnu)Sllog(solLum)stat.errorfloatnullablelog(nuLnu)Sm[10.3/12.5] Log of rest frame luminosity {nu}L_{nu}_ for steep-spectrum medium-z quasar typelog(solLum)phys.luminosityfloate_log(nuLnu)Sm[0.1/0.8]Uncertainty in log(nuLnu)Smlog(solLum)stat.errorfloatJ/AJ/151/120/table10Host Fit Parameters for the 3Cs at 0.5<z<1.0recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint3C[6.1/455] 3CR source name (3CNNN.N)meta.id;meta.mainfloatlogAHost[-15.72/-14.42] Log of the host galaxy fluxlog(W.m**-2)phot.fluxfloate_logAHost[0.03/0.23] Lower limit uncertainty in logAHostlog(W.m**-2)stat.errorfloatE_logAHost[0.03/0.27] Upper limit uncertainty in logAHostlog(W.m**-2)stat.error;stat.maxfloatZ[0.004/0.05] Metallicityphys.abund.Zfloatupsilon[6.9/10] Timescale {upsilon}log(yr)time.scalefloate_upsilon[0.3/2] Lower limit uncertainty in upsilonlog(yr)stat.errorfloatE_upsilon[0.3/2.2] Upper limit uncertainty in upsilonlog(yr)stat.error;stat.maxfloatlogAge[9.1/10] Log of the age of the stellar populationlog(yr)time.agefloate_logAge[0.04/0.3] Lower limit uncertainty in logAgelog(yr)stat.error;time.agefloatE_logAge[0.03/0.3] Upper limit uncertainty in logAgelog(yr)stat.error;stat.maxfloatM*[0.3/19] Stellar mass1e+11solMassphys.massfloate_M*[0.1/7.2] Lower limit uncertainty in M*1e+11solMassstat.errorfloatE_M*[0.1/19] Upper limit uncertainty in M*1e+11solMassstat.error;stat.maxfloatLHost[0.9/28] Luminosity of the host galaxy1e+11solLumphys.luminosityfloate_LHost[0.2/8.5] Lower limit uncertainty in LHost1e+11solLumstat.errorfloatE_LHost[0.2/8.4] Upper limit uncertainty in LHost1e+11solLumstat.error;stat.maxfloatMBH[3.8/428.7] Black hole mass1e+07solMassphys.massfloate_MBH[1.9/256.5] Lower limit uncertainty in MBH1e+07solMassstat.errorfloatE_MBH[2.6/1030.6] Upper limit uncertainty in MBH1e+07solMassstat.error;stat.maxfloatJ/AJ/151/120/table11Host Fit Parameters for the 3Cs at z<0.5Z[0.004/0.05] Metallicityphys.abund.ZfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint3C[20/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloatlogAHost[-15.14/-12.21] Log of the host galaxy fluxlog(W.m**-2)phot.fluxfloate_logAHost[0.01/0.24] Lower limit uncertainty in logAHostlog(W.m**-2)stat.errorfloatE_logAHost[0.01/0.17] Upper limit uncertainty in logAHostlog(W.m**-2)stat.error;stat.maxfloatupsilon[6.6/11] Timescale {upsilon}log(yr)time.scalefloate_upsilon[0.1/1.6] Lower limit uncertainty in upsilonlog(yr)stat.errorfloatE_upsilon[0.2/2.1] Upper limit uncertainty in upsilonlog(yr)stat.error;stat.maxfloatlogAge[9.1/10] Log of the age of the stellar populationlog(yr)time.agefloate_logAge[0.02/0.24] Lower limit uncertainty in logAgelog(yr)stat.error;time.agefloatE_logAge[0.01/0.3] Upper limit uncertainty in logAgelog(yr)stat.error;stat.maxfloatM*[0.4/210] Log of stellar mass1e+10solMassphys.massfloate_M*[0.2/65] Lower limit uncertainty in M*1e+10solMassstat.errorfloatE_M*[0.1/70] Upper limit uncertainty in M*1e+10solMassstat.error;stat.maxfloatLHost[0.5/170] Luminosity of the host galaxy1e+10solLumphys.luminosityfloate_LHost[0.1/44] Lower limit uncertainty in LHost1e+10solLumstat.errorfloatE_LHost[0.1/59] Upper limit uncertainty in LHost1e+10solLumstat.error;stat.maxfloatMBH[0.4/479.6] Black hole mass1e+07solMassphys.massfloate_MBH[0.2/265.3] Lower limit uncertainty in MBH1e+07solMassstat.errorfloatE_MBH[0.2/538.2] Upper limit uncertainty in MBH1e+07solMassstat.error;stat.maxfloatJ/AJ/151/120/table12AGN Fit Parameters for the 3Cs at 0.5<z<1.0e_LAGN[0.1/7.7] Lower limit uncertainty in LAGN1e+11solLumstat.errorfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint3C[6.1/455] 3CR source name (3CNNN.N)meta.id;meta.mainfloatlogAagn[-15.6/-14.11] Log of the AGN-heated warm dust fluxlog(W.m**-2)phot.fluxfloate_logAagn[0.02/0.22] Lower limit uncertainty in logAagnlog(W.m**-2)stat.errorfloatE_logAagn[0.01/0.12] Upper limit uncertainty in logAagnlog(W.m**-2)stat.error;stat.maxfloatInc[0/75] Inclination angle to the observerdegsrc.orbital.inclinationintNCloud[2.5/10] Number of clouds along the equatorial line of sightmeta.numberfloata[-2/0] Index of the power law for radial dust-cloud distributionmeta.code;spect.indexfloattheta[5/60] Half opening angle {theta}degpos.posAnginttau[30/80] Optical depth {tau}phys.absorption.opticalDepthintLAGN[0.9/56] AGN luminosity1e+11solLumphys.luminosityfloatE_LAGN[0.1/8.7] Upper limit uncertainty in LAGN1e+11solLumstat.error;stat.maxfloatLAGN/LEdd[0.0044/0.508] Ratio of AGN luminosity in the MIR and Eddington luminosity (G1)phys.luminosity;arith.ratiofloate_LAGN/LEdd[0.0021/0.2891] Lower limit uncertainty in LAGN/LEddstat.errorfloatE_LAGN/LEdd[0.0045/0.7034] Upper limit uncertainty in LAGN/LEddstat.error;stat.maxfloatJ/AJ/151/120/table13AGN Fit Parameters for the 3Cs at z<0.5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint3C[20/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloatlogAagn[-16.23/-12.89] Log of the AGN-heated warm dust fluxlog(W.m**-2)phot.fluxfloate_logAagn[0.01/0.27] Lower limit uncertainty in logAagnlog(W.m**-2)stat.errorfloatE_logAagn[0.01/0.23] Upper limit uncertainty in logAagnlog(W.m**-2)stat.error;stat.maxfloatInc[0/75] Inclination angle to the observerdegsrc.orbital.inclinationintNCloud[2.5/10] Number of clouds along the equatorial line of sightmeta.numberfloata[-2/0] Index of the power law for radial dust-cloud distributionmeta.code;spect.indexfloattheta[5/60] Half opening angle {theta}degpos.posAnginttau[30/80] Optical depth {tau}phys.absorption.opticalDepthintLAGN[0.1/3900] AGN luminosity1e+09solLumphys.luminosityfloate_LAGN[0.1/890] Lower limit uncertainty in LAGN1e+09solLumstat.errorfloatE_LAGN[0.1/580] Upper limit uncertainty in LAGN1e+09solLumstat.error;stat.maxfloatLAGN/LEdd[0.0001/0.6886] Ratio of AGN luminosity in the MIR and Eddington luminosity (G1)phys.luminosity;arith.ratiofloate_LAGN/LEdd[0.0001/0.3371] Lower limit uncertainty in LAGN/LEddstat.errorfloatE_LAGN/LEdd[0.0001/1.184] Upper limit uncertainty in LAGN/LEddstat.error;stat.maxfloatJ/AJ/151/120/table14FIR Fit Parameters for the 3Cs at 0.5<z<1.03C[6.1/455] 3CR source name (3CNNN.N)meta.id;meta.mainfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogAFIR[-15.59/-14.21] Log of the SF-heated cool dust fluxlog(W.m**-2)phot.fluxfloate_logAFIR[0.03/0.23] Lower limit uncertainty in logAFIRlog(W.m**-2)stat.errorfloatE_logAFIR[0.02/0.15] Upper limit uncertainty in logAFIRlog(W.m**-2)stat.error;stat.maxfloatTFIR[20/47] FIR dust temperatureKphys.temperaturefloate_TFIR[0.2/3.1] Lower limit uncertainty in TFIRKstat.errorfloatE_TFIR[0.2/3.1] Upper limit uncertainty in TFIRKstat.error;stat.maxfloatSFR[16.8/555.8] Star formation ratesolMass/yrphys.SFRfloate_SFR[1.4/83.4] Lower limit uncertainty in SFRsolMass/yrstat.error;phys.SFRfloatE_SFR[1.6/69.5] Upper limit uncertainty in SFRsolMass/yrstat.error;stat.maxfloatLFIR[1/32] Luminosity of cool FIR emitting dust1e+11solLumphys.luminosity;em.IRfloate_LFIR[0.1/4.8] Lower limit uncertainty in LFIR1e+11solLumstat.errorfloatE_LFIR[0.1/4] Upper limit uncertainty in LFIR1e+11solLumstat.error;stat.maxfloatMDust[1.85/264.41] Dust mass1e+07solMassphys.massfloate_MDust[0.13/125.32] Lower limit uncertainty in MDust1e+07solMassstat.errorfloatE_MDust[0.09/57.8] Upper limit uncertainty in MDust1e+07solMassstat.error;stat.maxfloatMDust/M*[0.017/8.814] Dust-to-stellar mass ratio in per mille unitsphys.mass;arith.ratiofloatJ/AJ/151/120/table15FIR Fit Parameters for the 3Cs at z<0.5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint3C[20/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloatlogAFIR[-15.7/-13.39] Log of the SF-heated cool dust fluxlog(W.m**-2)phot.fluxfloate_logAFIR[0.03/0.31] Lower limit uncertainty in logAFIRlog(W.m**-2)stat.errorfloatE_logAFIR[0.02/0.2] Upper limit uncertainty in logAFIRlog(W.m**-2)stat.error;stat.maxfloatTFIR[21/66] FIR dust temperatureKphys.temperaturefloate_TFIR[0.2/2.5] Lower limit uncertainty in TFIRKstat.errorfloatE_TFIR[0.2/2.5] Upper limit uncertainty in TFIRKstat.error;stat.maxfloatSFR[0.1/573.2] Star formation ratesolMass/yrphys.SFRfloate_SFR[0/55.6] Lower limit uncertainty in SFRsolMass/yrstat.error;phys.SFRfloatE_SFR[0/52.1] Upper limit uncertainty in SFRsolMass/yrstat.error;stat.maxfloatLFIR[0.3/3300] Luminosity of cool FIR emitting dust1e+09solLumphys.luminosity;em.IRfloate_LFIR[0.1/320] Lower limit uncertainty in LFIR1e+09solLumstat.errorfloatE_LFIR[0.2/300] Upper limit uncertainty in LFIR1e+09solLumstat.error;stat.maxfloatMDust[0.02/27.37] Dust mass1e+07solMassphys.massfloate_MDust[0/6.37] Lower limit uncertainty in MDust1e+07solMassstat.errorfloatE_MDust[0/4.26] Upper limit uncertainty in MDust1e+07solMassstat.error;stat.maxfloatMDust/M*[0.004/5.474] Dust-to-stellar mass ratio in per mille unitsphys.mass;arith.ratiofloatJ/AJ/151/120/table16Monochromatic Luminosities for the 3Cs at 0.5<z<1.0recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint3C[6.1/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloatlog(nuLnu)30GHz[7.21/11.6] Log of rest frame 30 GHz monochromatic luminosity {nu}L_{nu}_^30GHz^log(solLum)phys.luminosity;em.mm.30-50GHzfloate_log(nuLnu)30GHz[0.005/0.08] Uncertainty in log(nuLnu)30GHzlog(solLum)stat.errorfloatlog(nuLnu)178MHz[6.58/10.97] Log of rest frame 178 MHz monochromatic luminosity {nu}L_{nu}_^178MHz^log(solLum)phys.luminosity;em.radio.100-200MHzfloate_log(nuLnu)178MHz[0.001/0.065] Uncertainty in log(nuLnu)178MHzlog(solLum)stat.errorfloatlog(nuLnu)30um[7.98/12.34] Log of rest frame 30 {mu}m monochromatic luminosity {nu}L_{nu}_^30{mu}m^log(solLum)phys.luminosity;em.IR.15-30umfloate_log(nuLnu)30um[0.002/0.239] Uncertainty in log(nuLnu)30umlog(solLum)stat.errorfloatlog(nuLnu)60um[8.19/12.45] Log of rest frame 60 {mu}m monochromatic luminosity {nu}L_{nu}_^60{mu}m^log(solLum)phys.luminosity;em.IR.30-60umfloate_log(nuLnu)60um[0.001/0.137] Uncertainty in log(nuLnu)60umlog(solLum)stat.errorfloatlog(nuLnu)100um[8.44/12.31] Log of rest frame 100 {mu}m monochromatic luminosity {nu}L_{nu}_^100{mu}m^log(solLum)phys.luminosity;em.IR.60-100umfloate_log(nuLnu)100um[0.001/0.283] Uncertainty in log(nuLnu)100umlog(solLum)stat.errorfloatJ/AJ/151/120/table17Monochromatic Luminosities for the 3Cs at z<0.5recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint3C[6.1/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloatlog(nuLnu)30GHz[7.21/11.6] Log of rest frame 30 GHz monochromatic luminosity {nu}L_{nu}_^30GHz^log(solLum)phys.luminosity;em.mm.30-50GHzfloate_log(nuLnu)30GHz[0.005/0.08] Uncertainty in log(nuLnu)30GHzlog(solLum)stat.errorfloatlog(nuLnu)178MHz[6.58/10.97] Log of rest frame 178 MHz monochromatic luminosity {nu}L_{nu}_^178MHz^log(solLum)phys.luminosity;em.radio.100-200MHzfloate_log(nuLnu)178MHz[0.001/0.065] Uncertainty in log(nuLnu)178MHzlog(solLum)stat.errorfloatlog(nuLnu)30um[7.98/12.34] Log of rest frame 30 {mu}m monochromatic luminosity {nu}L_{nu}_^30{mu}m^log(solLum)phys.luminosity;em.IR.15-30umfloate_log(nuLnu)30um[0.002/0.239] Uncertainty in log(nuLnu)30umlog(solLum)stat.errorfloatlog(nuLnu)60um[8.19/12.45] Log of rest frame 60 {mu}m monochromatic luminosity {nu}L_{nu}_^60{mu}m^log(solLum)phys.luminosity;em.IR.30-60umfloate_log(nuLnu)60um[0.001/0.137] Uncertainty in log(nuLnu)60umlog(solLum)stat.errorfloatlog(nuLnu)100um[8.44/12.31] Log of rest frame 100 {mu}m monochromatic luminosity {nu}L_{nu}_^100{mu}m^log(solLum)phys.luminosity;em.IR.60-100umfloate_log(nuLnu)100um[0.001/0.283] Uncertainty in log(nuLnu)100umlog(solLum)stat.errorfloat