diff --git a/samples/vizier-catatalogue.xml b/samples/vizier-catatalogue.xml new file mode 100644 index 0000000..8442661 --- /dev/null +++ b/samples/vizier-catatalogue.xml @@ -0,0 +1,1058 @@ + + 2026-07-02T17:55:31Z-f + + +
+ ivo://CDS.VizieR/J/AJ/151/1202025-05-19T09:50:00Zivo_managedJ.AJ +
+ + + z<1 3CR radio galaxies and quasars star formationJ/AJ/151/120ivo://CDS.VizieR/J/AJ/151/120doi:10.26093/cds/vizier.51510120 + + CDS + + Westhues C. + + + Haas M. + + + Barthel P. + + + Wilkes B.J. + + + Willner S.P.,Kuraszkiewicz J. + + + Podigachoski P. + + + Leipski C. + + + Meisenheimer K.,Siebenmorgen R. + + + Chini R. + + 2021-12-16T13:37:06Z2018-04-11T12:15:26Z + + CDS support team
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
cds-question@unistra.fr + + + + radio-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/151/120CatalogResearch + + IsServedByTAP VizieR generic service + + + IsServedByConesearch service + + + related-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.html + + + https://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/151/120 + + + + + https://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+votable + + + + + https://tapvizier.cds.unistra.fr/TAPVizieR/tap + + + + Cone 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? + + TABLE + + + + + GET + text/xml+votable + + 180.050000true + + 4.12958379.2805560.005555555555555556 + + + + Cone 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? + + TABLE + + + + + GET + text/xml+votable + + 180.050000true + + 10.78833352.060.005555555555555556 + + + + 6/245 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=asciiInfraredRadio + + + + default + + J/AJ/151/120/table13CR Sources 0.5<z<1 Observed with Herschel + + z[0.0169/0.996] Redshiftsrc.redshift + + 0.51910.543340.75450.992980.996100.0 + + float + + + DL[66/6426] Luminosity distanceMpcpos.distance + + 2876.03029.744544.56397.56426.0100.0 + + int + + + TypeType of galaxy (2)src.classchar + + + PID[1/6] Proposal identifier (3)meta.codeint + + + SPObsID[1342229105/1342268340]? Herschel/SPIRE ObsIDmeta.id;obslongnullable + + + DEJ2000Degree of Declination (J2000)pos.eq.dec;meta.main + + + 3C[006.1/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloat + + + n_DEJ2000[c] Note on DEs (1)meta.notechar + + + n_Type[b,c d] Note(s) on Type (1)meta.notechar + + + PObsID4? Herschel/PACS fourth ObsIDmeta.id;obsnullable + + + SimbadNameSimbad column added by the CDSmeta.idcharnullable + + + RAJ2000Hour of Right Ascension (J2000)pos.eq.ra;meta.main + + + PObsID1? Herschel/PACS first ObsIDmeta.id;obsnullable + + + PObsID3? Herschel/PACS third ObsIDmeta.id;obsnullable + + + recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint + + + PObsID2? Herschel/PACS second ObsIDmeta.id;obsnullable + +
+ + J/AJ/151/120/table23CR Sources z<0.5 Observed with Herschel + + DL[66/6426] Luminosity distanceMpcpos.distance + + 66.097.0804.02329.02475.0100.0 + + int + + + z[0.0169/0.996] Redshiftsrc.redshift + + 0.01690.023750.1740.43650.458100.0 + + float + + + PObsID2? Herschel/PACS second ObsIDmeta.id;obsnullable + + + recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint + + + PObsID1? Herschel/PACS first ObsIDmeta.id;obsnullable + + + PObsID3? Herschel/PACS third ObsIDmeta.id;obsnullable + + + RAJ2000Hour of Right Ascension (J2000)pos.eq.ra;meta.main + + + SimbadNameSimbad column added by the CDSmeta.idcharnullable + + + PObsID4? Herschel/PACS fourth ObsIDmeta.id;obsnullable + + + n_Type[b,c d] Note(s) on Type (1)meta.notechar + + + DEJ2000Degree of Declination (J2000)pos.eq.dec;meta.main + + + SPObsID[1342229105/1342268340]? Herschel/SPIRE ObsIDmeta.id;obslongnullable + + + PID[1/6] Proposal identifier (3)meta.codeint + + + TypeType of galaxy (2)src.classchar + + + n_DEJ2000[c] Note on DEs (1)meta.notechar + + + 3C[006.1/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloat + +
+ + J/AJ/151/120/table43CR Sources 0.5<z<1 PACS and SPIRE Flux Densities + + F70[6/783]? Herschel/PACS 70 {mu}m flux densitymJyphot.flux.density;em.IR.30-60um + + 6.06.10999999999999915.077.990.097.44 + + intnullable + + + F500[23/1062]? Herschel/SPIRE 500{mu}m flux densitymJyphot.flux.density;em.mm.400-750GHz + + 23.023.042.0263.69266.030.77 + + intnullable + + + F100[6/867]? Herschel/PACS 100 {mu}m flux densitymJyphot.flux.density;em.IR.60-100um + + 6.07.85999999999999919.0103.68126.082.05 + + intnullable + + + F160[13/1347]? Herschel/PACS 160 {mu}m flux densitymJyphot.flux.density;em.mm.1500-3000GHz + + 13.018.027.0148.16259.0100.0 + + intnullable + + + F250[22/955]? Herschel/SPIRE 250 {mu}m flux densitymJyphot.flux.density;em.mm.750-1500GHz + + 31.031.051.0370.15999999999997452.030.77 + + intnullable + + + F350[20/741]? Herschel/SPIRE 350 {mu}m flux densitymJyphot.flux.density;em.mm.750-1500GHz + + 22.025.343.5351.61412.030.77 + + intnullable + + + e_F100[1/6]? 1{sigma} uncertainty in F100mJystat.errorintnullable + + + l_F100[<] Limit flag on F100meta.code.errorchar + + + 3C[006.1/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloat + + + l_F160[<] Limit flag on F160meta.code.errorchar + + + l_F70[<] Limit flag on F70meta.code.errorchar + + + e_F250[8/27]? 1{sigma} uncertainty in F250mJystat.errorintnullable + + + e_F500[7/31]? 1{sigma} uncertainty in F500mJystat.errorintnullable + + + l_F250[<] Limit flag on F250meta.code.errorchar + + + l_F500[<] Limit flag on F500meta.code.errorchar + + + Fig[1/15] Figure number in the papermeta.idint + + + e_F160[3/24]? 1{sigma} uncertainty in F160mJystat.errorintnullable + + + e_F350[8/26]? 1{sigma} uncertainty in F350mJystat.errorintnullable + + + recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint + + + e_F70[2/8]? 1{sigma} uncertainty in F70mJystat.errorintnullable + + + l_F350[<] Limit flag on F350meta.code.errorchar + +
+ + J/AJ/151/120/table53CR Sources z<0.5 PACS and SPIRE Flux Densities + + F250[22/955]? Herschel/SPIRE 250 {mu}m flux densitymJyphot.flux.density;em.mm.750-1500GHz + + 22.023.3290.0743.14955.047.92 + + intnullable + + + F350[20/741]? Herschel/SPIRE 350 {mu}m flux densitymJyphot.flux.density;em.mm.750-1500GHz + + 20.024.61999999999999751.0702.72741.047.92 + + intnullable + + + F100[6/867]? Herschel/PACS 100 {mu}m flux densitymJyphot.flux.density;em.IR.60-100um + + 7.08.231.0543.3999999999994867.085.42 + + intnullable + + + F160[13/1347]? Herschel/PACS 160 {mu}m flux densitymJyphot.flux.density;em.mm.1500-3000GHz + + 13.016.5237.0990.04000000000121347.089.58 + + intnullable + + + F70[6/783]? Herschel/PACS 70 {mu}m flux densitymJyphot.flux.density;em.IR.30-60um + + 6.06.028.0292.9599999999998783.072.92 + + intnullable + + + F500[23/1062]? Herschel/SPIRE 500{mu}m flux densitymJyphot.flux.density;em.mm.400-750GHz + + 23.023.044.0939.241062.047.92 + + intnullable + + + 3C[006.1/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloat + + + e_F250[8/27]? 1{sigma} uncertainty in F250mJystat.errorintnullable + + + l_F70[<] Limit flag on F70meta.code.errorchar + + + l_F160[<] Limit flag on F160meta.code.errorchar + + + e_F100[1/6]? 1{sigma} uncertainty in F100mJystat.errorintnullable + + + l_F100[<] Limit flag on F100meta.code.errorchar + + + l_F350[<] Limit flag on F350meta.code.errorchar + + + e_F70[2/8]? 1{sigma} uncertainty in F70mJystat.errorintnullable + + + e_F500[7/31]? 1{sigma} uncertainty in F500mJystat.errorintnullable + + + recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint + + + e_F350[8/26]? 1{sigma} uncertainty in F350mJystat.errorintnullable + + + e_F160[3/24]? 1{sigma} uncertainty in F160mJystat.errorintnullable + + + Fig[1/15] Figure number in the papermeta.idint + + + l_F500[<] Limit flag on F500meta.code.errorchar + + + l_F250[<] Limit flag on F250meta.code.errorchar + +
+ + J/AJ/151/120/table6Median Spectral Templates for Different Galaxy Types Separated for Low- (z<0.5) and Medium-redshift (0.5<z<1) + + log(nuLnu)Hl[8.7/11.1] Log of rest frame luminosity {nu}L_{nu}_ for high-excitation radio low-z galaxy typelog(solLum)phys.luminosity + + 8.78.81710.611.011.1100.0 + + float + + + log(nuLnu)L[8.7/11.2]? Log of rest frame luminosity {nu}L_{nu}_ for low-excitation radio galaxy typelog(solLum)phys.luminosity + + 8.78.8149.611.111.297.5 + + floatnullable + + + log(nuLnu)Sl[10.2/12.2]? Log of rest frame luminosity {nu}L_{nu}_ for steep-spectrum low-z quasar typelog(solLum)phys.luminosity + + 10.210.29900000000000111.712.10099999999999912.285.0 + + floatnullable + + + log(nuLnu)B[9.1/11.5]? Log of rest frame luminosity {nu}L_{nu}_ for broad-line radio galaxy typelog(solLum)phys.luminosity + + 9.19.21399999999999911.011.511.597.5 + + floatnullable + + + log(nuLnu)Fl[8.4/11]? Log of rest frame luminosity {nu}L_{nu}_ for flat-spectrum low-z quasar typelog(solLum)phys.luminosity + + 8.48.82500000000000110.5511.011.090.0 + + floatnullable + + + log(nuLnu)Sm[10.3/12.5] Log of rest frame luminosity {nu}L_{nu}_ for steep-spectrum medium-z quasar typelog(solLum)phys.luminosity + + 10.310.412.012.48312.5100.0 + + float + + + log(nuLnu)Hm[10/11.5] Log of rest frame luminosity {nu}L_{nu}_ for high-excitation radio medium-z galaxy typelog(solLum)phys.luminosity + + 10.010.11699999999999911.0511.411.5100.0 + + float + + + log(nuLnu)Fm[10.2/12.1]? Log of rest frame luminosity {nu}L_{nu}_ for flat-spectrum medium-z quasar typelog(solLum)phys.luminosity + + 10.210.41411.812.08612.197.5 + + floatnullable + + + e_log(nuLnu)Hl[0.1/1] Uncertainty in log(nuLnu)Hllog(solLum)stat.errorfloat + + + e_log(nuLnu)B[0.1/0.9]? Uncertainty in log(nuLnu)Blog(solLum)stat.errorfloatnullable + + + e_log(nuLnu)L[0.1/1.3]? Uncertainty in log(nuLnu)Llog(solLum)stat.errorfloatnullable + + + log(lrest)[-0.4/6.6] Log of rest wavelength {lambda}_Rest_log(um)em.wlfloat + + + e_log(nuLnu)Sl[0.2/1.6]? Uncertainty in log(nuLnu)Sllog(solLum)stat.errorfloatnullable + + + e_log(nuLnu)Fm[0.2/0.3]? Uncertainty in log(nuLnu)Fmlog(solLum)stat.errorfloatnullable + + + e_log(nuLnu)Hm[0.1/0.7] Uncertainty in log(nuLnu)Hmlog(solLum)stat.errorfloat + + + e_log(nuLnu)Fl[0.3/0.8]? Uncertainty in log(nuLnu)Fllog(solLum)stat.errorfloatnullable + + + e_log(nuLnu)Sm[0.1/0.8]Uncertainty in log(nuLnu)Smlog(solLum)stat.errorfloat + + + recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint + +
+ + J/AJ/151/120/table10Host Fit Parameters for the 3Cs at 0.5<z<1.0 + + M*[0.3/19] Stellar mass1e+11solMassphys.mass + + 0.300000000000000040.75600000000000013.700000000000000617.58000000000000219.000000000000004100.0 + + float + + + LHost[0.9/28] Luminosity of the host galaxy1e+11solLumphys.luminosity + + 0.90000000000000011.27000000000000024.90000000000000125.72000000000000228.000000000000007100.0 + + float + + + MBH[3.8/428.7] Black hole mass1e+07solMassphys.mass + + 3.811.14999999999999968.6393.15599999999995428.7100.0 + + float + + + E_logAge[0.03/0.3] Upper limit uncertainty in logAgelog(yr)stat.error;stat.maxfloat + + + recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint + + + E_LHost[0.2/8.4] Upper limit uncertainty in LHost1e+11solLumstat.error;stat.maxfloat + + + e_logAge[0.04/0.3] Lower limit uncertainty in logAgelog(yr)stat.error;time.agefloat + + + logAHost[-15.72/-14.42] Log of the host galaxy fluxlog(W.m**-2)phot.fluxfloat + + + E_MBH[2.6/1030.6] Upper limit uncertainty in MBH1e+07solMassstat.error;stat.maxfloat + + + e_MBH[1.9/256.5] Lower limit uncertainty in MBH1e+07solMassstat.errorfloat + + + e_M*[0.1/7.2] Lower limit uncertainty in M*1e+11solMassstat.errorfloat + + + Z[0.004/0.05] Metallicityphys.abund.Zfloat + + + upsilon[6.9/10] Timescale {upsilon}log(yr)time.scalefloat + + + E_upsilon[0.3/2.2] Upper limit uncertainty in upsilonlog(yr)stat.error;stat.maxfloat + + + e_logAHost[0.03/0.23] Lower limit uncertainty in logAHostlog(W.m**-2)stat.errorfloat + + + E_M*[0.1/19] Upper limit uncertainty in M*1e+11solMassstat.error;stat.maxfloat + + + logAge[9.1/10] Log of the age of the stellar populationlog(yr)time.agefloat + + + e_upsilon[0.3/2] Lower limit uncertainty in upsilonlog(yr)stat.errorfloat + + + e_LHost[0.2/8.5] Lower limit uncertainty in LHost1e+11solLumstat.errorfloat + + + E_logAHost[0.03/0.27] Upper limit uncertainty in logAHostlog(W.m**-2)stat.error;stat.maxfloat + + + 3C[6.1/455] 3CR source name (3CNNN.N)meta.id;meta.mainfloat + +
+ + J/AJ/151/120/table11Host Fit Parameters for the 3Cs at z<0.5 + + LHost[0.5/170] Luminosity of the host galaxy1e+10solLumphys.luminosity + + 0.49999999999999992.281999999999999611.499999999999998135.89999999999992169.99999999999997100.0 + + float + + + M*[0.4/210] Log of stellar mass1e+10solMassphys.mass + + 0.41.2468.569.94999999999999210.0100.0 + + float + + + MBH[0.4/479.6] Black hole mass1e+07solMassphys.mass + + 0.41.52813.2140.00799999999995479.6100.0 + + float + + + upsilon[6.6/11] Timescale {upsilon}log(yr)time.scalefloat + + + E_upsilon[0.2/2.1] Upper limit uncertainty in upsilonlog(yr)stat.error;stat.maxfloat + + + e_logAHost[0.01/0.24] Lower limit uncertainty in logAHostlog(W.m**-2)stat.errorfloat + + + E_M*[0.1/70] Upper limit uncertainty in M*1e+10solMassstat.error;stat.maxfloat + + + logAge[9.1/10] Log of the age of the stellar populationlog(yr)time.agefloat + + + e_upsilon[0.1/1.6] Lower limit uncertainty in upsilonlog(yr)stat.errorfloat + + + e_LHost[0.1/44] Lower limit uncertainty in LHost1e+10solLumstat.errorfloat + + + E_logAHost[0.01/0.17] Upper limit uncertainty in logAHostlog(W.m**-2)stat.error;stat.maxfloat + + + 3C[20/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloat + + + E_logAge[0.01/0.3] Upper limit uncertainty in logAgelog(yr)stat.error;stat.maxfloat + + + E_LHost[0.1/59] Upper limit uncertainty in LHost1e+10solLumstat.error;stat.maxfloat + + + recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint + + + e_logAge[0.02/0.24] Lower limit uncertainty in logAgelog(yr)stat.error;time.agefloat + + + logAHost[-15.14/-12.21] Log of the host galaxy fluxlog(W.m**-2)phot.fluxfloat + + + E_MBH[0.2/538.2] Upper limit uncertainty in MBH1e+07solMassstat.error;stat.maxfloat + + + e_MBH[0.2/265.3] Lower limit uncertainty in MBH1e+07solMassstat.errorfloat + + + e_M*[0.2/65] Lower limit uncertainty in M*1e+10solMassstat.errorfloat + + + Z[0.004/0.05] Metallicityphys.abund.Zfloat + +
+ + J/AJ/151/120/table12AGN Fit Parameters for the 3Cs at 0.5<z<1.0 + + tau[30/80] Optical depth {tau}phys.absorption.opticalDepth + + 30.030.050.050.080.0100.0 + + int + + + LAGN[0.9/56] AGN luminosity1e+11solLumphys.luminosity + + 0.90000000000000011.09816.00000000000000452.58000000000000556.000000000000014100.0 + + float + + + LAGN/LEdd[0.0044/0.508] Ratio of AGN luminosity in the MIR and Eddington luminosity (G1)phys.luminosity;arith.ratio + + 0.00440.0050459999999999990.05370.334481999999999950.508100.0 + + float + + + Inc[0/75] Inclination angle to the observerdegsrc.orbital.inclinationint + + + E_LAGN/LEdd[0.0045/0.7034] Upper limit uncertainty in LAGN/LEddstat.error;stat.maxfloat + + + logAagn[-15.6/-14.11] Log of the AGN-heated warm dust fluxlog(W.m**-2)phot.fluxfloat + + + E_LAGN[0.1/8.7] Upper limit uncertainty in LAGN1e+11solLumstat.error;stat.maxfloat + + + recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint + + + e_LAGN[0.1/7.7] Lower limit uncertainty in LAGN1e+11solLumstat.errorfloat + + + 3C[6.1/455] 3CR source name (3CNNN.N)meta.id;meta.mainfloat + + + E_logAagn[0.01/0.12] Upper limit uncertainty in logAagnlog(W.m**-2)stat.error;stat.maxfloat + + + a[-2/0] Index of the power law for radial dust-cloud distributionmeta.code;spect.indexfloat + + + e_LAGN/LEdd[0.0021/0.2891] Lower limit uncertainty in LAGN/LEddstat.errorfloat + + + e_logAagn[0.02/0.22] Lower limit uncertainty in logAagnlog(W.m**-2)stat.errorfloat + + + theta[5/60] Half opening angle {theta}degpos.posAngint + + + NCloud[2.5/10] Number of clouds along the equatorial line of sightmeta.numberfloat + +
+ + J/AJ/151/120/table13AGN Fit Parameters for the 3Cs at z<0.5 + + LAGN/LEdd[0.0001/0.6886] Ratio of AGN luminosity in the MIR and Eddington luminosity (G1)phys.luminosity;arith.ratio + + 0.00010.0001410.01110.478395999999999040.6886100.0 + + float + + + tau[30/80] Optical depth {tau}phys.absorption.opticalDepth + + 30.030.030.050.080.0100.0 + + int + + + LAGN[0.1/3900] AGN luminosity1e+09solLumphys.luminosity + + 0.100000000000000020.582000000000000145.500000000000013518.03900.000000000001100.0 + + float + + + NCloud[2.5/10] Number of clouds along the equatorial line of sightmeta.numberfloat + + + theta[5/60] Half opening angle {theta}degpos.posAngint + + + a[-2/0] Index of the power law for radial dust-cloud distributionmeta.code;spect.indexfloat + + + e_logAagn[0.01/0.27] Lower limit uncertainty in logAagnlog(W.m**-2)stat.errorfloat + + + e_LAGN/LEdd[0.0001/0.3371] Lower limit uncertainty in LAGN/LEddstat.errorfloat + + + 3C[20/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloat + + + E_logAagn[0.01/0.23] Upper limit uncertainty in logAagnlog(W.m**-2)stat.error;stat.maxfloat + + + E_LAGN[0.1/580] Upper limit uncertainty in LAGN1e+09solLumstat.error;stat.maxfloat + + + logAagn[-16.23/-12.89] Log of the AGN-heated warm dust fluxlog(W.m**-2)phot.fluxfloat + + + e_LAGN[0.1/890] Lower limit uncertainty in LAGN1e+09solLumstat.errorfloat + + + recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint + + + Inc[0/75] Inclination angle to the observerdegsrc.orbital.inclinationint + + + E_LAGN/LEdd[0.0001/1.184] Upper limit uncertainty in LAGN/LEddstat.error;stat.maxfloat + +
+ + J/AJ/151/120/table14FIR Fit Parameters for the 3Cs at 0.5<z<1.0 + + LFIR[1/32] Luminosity of cool FIR emitting dust1e+11solLumphys.luminosity;em.IR + + 1.00000000000000021.20000000000000024.80000000000000120.72000000000000232.00000000000001100.0 + + float + + + TFIR[20/47] FIR dust temperatureKphys.temperature + + 20.021.1432.042.8647.0100.0 + + float + + + MDust[1.85/264.41] Dust mass1e+07solMassphys.mass + + 1.85000000000000032.163416.17226.97799999999998264.41100.0 + + float + + + MDust/M*[0.017/8.814] Dust-to-stellar mass ratio in per mille unitsphys.mass;arith.ratio + + 0.0170.061999999999999990.374.13507999999999858.814100.0 + + float + + + logAFIR[-15.59/-14.21] Log of the SF-heated cool dust fluxlog(W.m**-2)phot.fluxfloat + + + e_LFIR[0.1/4.8] Lower limit uncertainty in LFIR1e+11solLumstat.errorfloat + + + E_SFR[1.6/69.5] Upper limit uncertainty in SFRsolMass/yrstat.error;stat.maxfloat + + + recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint + + + E_LFIR[0.1/4] Upper limit uncertainty in LFIR1e+11solLumstat.error;stat.maxfloat + + + e_MDust[0.13/125.32] Lower limit uncertainty in MDust1e+07solMassstat.errorfloat + + + e_TFIR[0.2/3.1] Lower limit uncertainty in TFIRKstat.errorfloat + + + SFR[16.8/555.8] Star formation ratesolMass/yrphys.SFRfloat + + + E_TFIR[0.2/3.1] Upper limit uncertainty in TFIRKstat.error;stat.maxfloat + + + e_SFR[1.4/83.4] Lower limit uncertainty in SFRsolMass/yrstat.error;phys.SFRfloat + + + e_logAFIR[0.03/0.23] Lower limit uncertainty in logAFIRlog(W.m**-2)stat.errorfloat + + + 3C[6.1/455] 3CR source name (3CNNN.N)meta.id;meta.mainfloat + + + E_logAFIR[0.02/0.15] Upper limit uncertainty in logAFIRlog(W.m**-2)stat.error;stat.maxfloat + + + E_MDust[0.09/57.8] Upper limit uncertainty in MDust1e+07solMassstat.error;stat.maxfloat + +
+ + J/AJ/151/120/table15FIR Fit Parameters for the 3Cs at z<0.5 + + LFIR[0.3/3300] Luminosity of cool FIR emitting dust1e+09solLumphys.luminosity;em.IR + + 0.300000000000000041.100000000000000321.000000000000004746.49999999999893300.0000000000005100.0 + + float + + + TFIR[21/66] FIR dust temperatureKphys.temperature + + 21.021.4130.047.58999999999999666.0100.0 + + float + + + MDust[0.02/27.37] Dust mass1e+07solMassphys.mass + + 0.020.03410.91519.66079999999994527.37100.0 + + float + + + MDust/M*[0.004/5.474] Dust-to-stellar mass ratio in per mille unitsphys.mass;arith.ratio + + 0.0040.005410.111.5867999999999975.474100.0 + + float + + + logAFIR[-15.7/-13.39] Log of the SF-heated cool dust fluxlog(W.m**-2)phot.fluxfloat + + + e_LFIR[0.1/320] Lower limit uncertainty in LFIR1e+09solLumstat.errorfloat + + + E_SFR[0/52.1] Upper limit uncertainty in SFRsolMass/yrstat.error;stat.maxfloat + + + recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint + + + E_LFIR[0.2/300] Upper limit uncertainty in LFIR1e+09solLumstat.error;stat.maxfloat + + + e_MDust[0/6.37] Lower limit uncertainty in MDust1e+07solMassstat.errorfloat + + + SFR[0.1/573.2] Star formation ratesolMass/yrphys.SFRfloat + + + e_TFIR[0.2/2.5] Lower limit uncertainty in TFIRKstat.errorfloat + + + 3C[20/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloat + + + E_logAFIR[0.02/0.2] Upper limit uncertainty in logAFIRlog(W.m**-2)stat.error;stat.maxfloat + + + E_MDust[0/4.26] Upper limit uncertainty in MDust1e+07solMassstat.error;stat.maxfloat + + + E_TFIR[0.2/2.5] Upper limit uncertainty in TFIRKstat.error;stat.maxfloat + + + e_SFR[0/55.6] Lower limit uncertainty in SFRsolMass/yrstat.error;phys.SFRfloat + + + e_logAFIR[0.03/0.31] Lower limit uncertainty in logAFIRlog(W.m**-2)stat.errorfloat + +
+ + J/AJ/151/120/table16Monochromatic Luminosities for the 3Cs at 0.5<z<1.0 + + log(nuLnu)178MHz[6.58/10.97] Log of rest frame 178 MHz monochromatic luminosity {nu}L_{nu}_^178MHz^log(solLum)phys.luminosity;em.radio.100-200MHz + + 9.749.751410.1610.730210.97100.0 + + float + + + log(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.15-30um + + 10.5110.814211.712.305812.34100.0 + + float + + + log(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.30-60um + + 10.7210.855211.6312.27179999999999912.34100.0 + + float + + + log(nuLnu)30GHz[7.21/11.6] Log of rest frame 30 GHz monochromatic luminosity {nu}L_{nu}_^30GHz^log(solLum)phys.luminosity;em.mm.30-50GHz + + 9.9210.011410.4711.46300000000000111.6100.0 + + float + + + log(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.60-100um + + 10.910.909811.5912.087212.23100.0 + + float + + + recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint + + + e_log(nuLnu)100um[0.001/0.283] Uncertainty in log(nuLnu)100umlog(solLum)stat.errorfloat + + + e_log(nuLnu)178MHz[0.001/0.065] Uncertainty in log(nuLnu)178MHzlog(solLum)stat.errorfloat + + + e_log(nuLnu)30um[0.002/0.239] Uncertainty in log(nuLnu)30umlog(solLum)stat.errorfloat + + + e_log(nuLnu)60um[0.001/0.137] Uncertainty in log(nuLnu)60umlog(solLum)stat.errorfloat + + + e_log(nuLnu)30GHz[0.005/0.08] Uncertainty in log(nuLnu)30GHzlog(solLum)stat.errorfloat + + + 3C[6.1/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloat + +
+ + J/AJ/151/120/table17Monochromatic Luminosities for the 3Cs at z<0.5 + + log(nuLnu)30GHz[7.21/11.6] Log of rest frame 30 GHz monochromatic luminosity {nu}L_{nu}_^30GHz^log(solLum)phys.luminosity;em.mm.30-50GHz + + 7.217.37179.18499999999999910.44179999999999910.99100.0 + + float + + + log(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.60-100um + + 8.448.84940000000000110.2111.626712.31100.0 + + float + + + log(nuLnu)178MHz[6.58/10.97] Log of rest frame 178 MHz monochromatic luminosity {nu}L_{nu}_^178MHz^log(solLum)phys.luminosity;em.radio.100-200MHz + + 6.586.76928.839.88590000000000110.05100.0 + + float + + + log(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.15-30um + + 7.988.644110.37512.057712.33100.0 + + float + + + log(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.30-60um + + 8.198.809210.28000000000000111.85179999999999912.45100.0 + + float + + + e_log(nuLnu)60um[0.001/0.137] Uncertainty in log(nuLnu)60umlog(solLum)stat.errorfloat + + + e_log(nuLnu)30um[0.002/0.239] Uncertainty in log(nuLnu)30umlog(solLum)stat.errorfloat + + + e_log(nuLnu)30GHz[0.005/0.08] Uncertainty in log(nuLnu)30GHzlog(solLum)stat.errorfloat + + + 3C[6.1/459] 3CR source name (3CNNN.N)meta.id;meta.mainfloat + + + e_log(nuLnu)178MHz[0.001/0.065] Uncertainty in log(nuLnu)178MHzlog(solLum)stat.errorfloat + + + e_log(nuLnu)100um[0.001/0.283] Uncertainty in log(nuLnu)100umlog(solLum)stat.errorfloat + + + recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint + +
+ + + + + + +