VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
Target Name (resolved by Sesame) or Position:
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NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/MNRAS/512/86
  ISM study with nearby AGNs and galaxies (Bernhard+, 2022)
Post annotation
img(gal)
1.J/MNRAS/512/86/2jytab1(c)*Properties and dust masses derived with 100/160 microns flux ratios method of the 2Jy sample (Note) (46 rows)
2.J/MNRAS/512/86/3crtab1(c)*Properties and dust masses derived with 100/160 microns flux ratios method of the 3CR sample (Note) (45 rows)
3.J/MNRAS/512/86/atlatab1(c)*Properties and dust masses derived with 100/160 microns flux ratios method of the Atlas3D sample (Note) (6 rows)
4.J/MNRAS/512/86/hrstab1(c)*Properties and dust masses derived with 100/160 microns flux ratios method of the HRS sample (Note) (8 rows)
5.J/MNRAS/512/86/pgqtab1(c)*Properties and dust masses derived with 100/160 microns flux ratios method of the PG QSO sample (Note) (70 rows)
6.J/MNRAS/512/86/t2qstab1(c)*Properties and dust masses derived with 100/160 microns flux ratios method of Type-II QSO sample (Note) (86 rows)
7.J/MNRAS/512/86/ulirtab1(c)*Properties and dust masses derived with 100/160 microns flux ratios method of the ULIRG sample (Note) (41 rows)
8.J/MNRAS/512/86/2jytab2*Properties and dust masses derived with IR SED fits method of the 2Jy sample (Note) (8 rows)
9.J/MNRAS/512/86/3crtab2*Properties and dust masses derived with IR SED fits method of the 3CR sample (Note) (4 rows)
10.J/MNRAS/512/86/atlatab2*Properties and dust masses derived with IR SED fits method of the Atlas3D sample (Note) (3 rows)
11.J/MNRAS/512/86/pgqtab2*Properties and dust masses derived with IR SED fits method of the PG QSO sample (Note) (9 rows)
12.J/MNRAS/512/86/t2qstab2*Properties and dust masses derived with IR SED fits method of the Type-II QSO sample (Note) (12 rows)
13.J/MNRAS/512/86/ulirtab2*Properties and dust masses derived with IR SED fits method of the ULIRG sample (Note) (14 rows)
14.J/MNRAS/512/86/2jytab3*K-band stellar mass and SFRs for the 2Jy sample (Note) (46 rows)
15.J/MNRAS/512/86/3crtab3*K-band stellar mass and SFRs for the 3CR sample (Note) (45 rows)
16.J/MNRAS/512/86/atlatab3*K-band stellar mass and SFRs for Atlas3D sample (Note) (6 rows)
17.J/MNRAS/512/86/hrstab3*K-band stellar mass and SFRs for the HRS sample (Note) (8 rows)
18.J/MNRAS/512/86/pgqtab3*K-band stellar mass and SFRs for PG QSO sample (Note) (70 rows)
19.J/MNRAS/512/86/t2qstab3*K-band stellar mass and SFRs for Type-II QSO sample (Note) (86 rows)
20.J/MNRAS/512/86/ulirtab3*K-band stellar mass and SFRs for ULIRG sample (Note) (41 rows)

 
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
   (1+2+3+5+6+7)tab2 (char) Indicates properties and dust masses derived by IR SED fits in tab2 (meta.ref.url)
   (ALL)Name (char) (i) Name identification of the source (ID) (meta.id;meta.main)
  (1+2+3+4+5+6+7)RAJ2000 deg (i) Right Ascension (J2000) (RA_deg) (pos.eq.ra;meta.main)
  (1+2+3+4+5+6+7)DEJ2000 deg (i) Declination (J2000) (DEC_deg) (pos.eq.dec;meta.main)
  (1+2+3+4+5+6+7)z  Redshift (z) (src.redshift)
  (1+2+3+4+5+6+7)Classrad (char) Radio classification only for the 91 radio AGN objects (rad_class) (Note 1)   (meta.code.class)
  (1+2+3+4+5+6+7)Classopt (char) Optical classification only for 91 radio AGN objects (opt_class) (Note 2)   (meta.code.class)
  (1+2+3+4+5+6+7)L[OIII] [W] (n) The [OIII] 5007 Å luminosity only for AGN objects (LOIII_W) (phys.luminosity;em.line.OIII)
  (1+2+3+4+5+6+7+8+9+10+11+12+13)logBnuTCNorm [-] Log-normalisation of the cold component of the black body curve obtained with the TC model (logNorm_TC) (Note 3)   (phot.flux.density;em.mm.1500-3000GHz;arith.ratio)
  (1+2+3+4+5+6+7+8+9+10+11+12+13)e_logBnuTCNorm [-] Mean uncertainty of logBnuTCNorm (elogNorm_TC) (stat.error)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3+4+5+6+7+8+9+10+11+12+13)TcoldTC K Temperature of the cool dust component obtained with the TC model (T_TC) (Note 3)   (phys.temperature;meta.modelled)
  (1+2+3+4+5+6+7+8+9+10+11+12+13)e_TcoldTC K Mean uncertainty of TcoldTC (eT_TC) (stat.error)
  (1+2+3+4+5+6+7+8+9+10+11+12+13)BetaTC  Beta index of the modified black body obtained with the TC model (beta_TC) (Note 3)   (spect.index;meta.modelled)
  (1+2+3+4+5+6+7+8+9+10+11+12+13)e_BetaTC  Mean uncertainty of BetaTC (ebeta_TC) (stat.error)
  (1+2+3+4+5+6+7+8+9+10+11+12+13)logBnuTCBFNorm [-] Log-normalisation of the cold component of the black body curve obtained with the TCBF model (logNorm_TCBF) (Note 4)   (phot.flux.density;em.mm.1500-3000GHz;arith.ratio)
  (1+2+3+4+5+6+7+8+9+10+11+12+13)e_logBnuTCBFNorm [-] Mean uncertainty of logBnuTCBFNorm (elogNorm_TCBF) (stat.error)
  (1+2+3+4+5+6+7+8+9+10+11+12+13)TcoldTCBF K Temperature of the cool dust component obtained with the TCBF model (T_TCBF) (Note 4)   (phys.temperature;meta.modelled)
  (1+2+3+4+5+6+7+8+9+10+11+12+13)e_TcoldTCBF K Mean uncertainty of TcoldTCBF (eT_TCBF) (stat.error)
  (1+2+3+4+5+6+7+8+9+10+11+12+13)BetaTCBF  Beta index of the modified black body fixed to 2 with the TCBF model (beta_TCBF) (Note 4)   (spect.index;meta.modelled)
  (1+2+3+4+5+6+7+8+9+10+11+12+13)logMdustTC [Msun] The log of the dust mass calculated using TC model (logMdust_TC) (Note 3)   (phys.mass;meta.modelled)
  (1+2+3+4+5+6+7+8+9+10+11+12+13)e_logMdustTC [Msun] (n) Mean uncertainty of logMdustTC (elogMdust_TC) (stat.error)
  (1+2+3+4+5+6+7+8+9+10+11+12+13)logMdustTCBF [Msun] The log of the dust mass calculated using TCBF model (logMdust_TCBF) (Note 4)   (phys.mass;meta.modelled)
  (1+2+3+4+5+6+7+8+9+10+11+12+13)e_logMdustTCBF [Msun] (n) Mean uncertainty of logMdustTCBF (elogMdust_TCBF) (stat.error)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+3+4)Simbad (char) ask the Simbad data-base about this object (meta.ref.url)
  (2+5+6+7)SimbadName (char) (n)Designation understandable by the Simbad data-base (meta.id)
  (8+9+10+11+12+13)logBnuOCNorm [-] Log-normalisation of the cold component of the black body curve obtained with the OC model (logNorm_OC) (Note 1)   (phot.flux.density;em.mm.1500-3000GHz;arith.ratio)
  (8+9+10+11+12+13)e_logBnuOCNorm [-] Mean uncertainty of logBnuOCNorm (elogNorm_OC) (stat.error)
  (8+9+10+11+12+13)TcoldOC K Temperature of the cool dust component obtained with the OC model (T_OC) (Note 1)   (phys.temperature;meta.modelled)
  (8+9+10+11+12+13)e_TcoldOC K Mean uncertainty of TcoldOC (eT_OC) (stat.error)
  (8+9+10+11+12+13)BetaOC  Beta index of the modified black body obtained with the OC model (beta_OC) (Note 1)   (spect.index;meta.modelled)
  (8+9+10+11+12+13)e_BetaOC  Mean uncertainty of BetaOC (ebeta_OC) (stat.error)
  (14+15+16+17+18+19+20)logM* [Msun] (n) Stellar mass estimated converting the K-band luminosities using M/L ratios (logMstar) (phys.mass;meta.modelled)
  (14+15+16+17+18+19+20)e_logM* [Msun] (n) Mean uncertainty of logM* (elogMstar) (stat.error)
  (14+15+16+17+18+19+20)f_logM*  (n) Flag indicating the method used to calculate stellar masses (Mstar_flag) (Note 1)   (meta.code)
  (14+15+16+17+18+19+20)SFR Msun/yr Star formation rate computed with IRAGNSEP decomposes IR SEDs into an AGN and a galaxy contributions (SFR) (phys.SFR;meta.modelled)
  (14+15+16+17+18+19+20)e_SFR Msun/yr (n) Mean uncertainty on SFR (eSFR) (stat.error;phys.SFR)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
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