VizieR

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

VizieR

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J/MNRAS/472/334
  Optical/MIR properties of Type 1 AGNs (Lakicevic+, 2017)
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2017MNRAS.472..334L
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Post annotation 		img(gal)
1.J/MNRAS/472/334/table1(c)The sample of Type 1 AGNs, observed at the MIR and optical wavelengths[spectrum] (82 rows)
2.J/MNRAS/472/334/table2The sample of Type 2 AGNs taken from the literature and the data that have been used in this work (49 rows)
3.J/MNRAS/472/334/table3The optical parameters that we measured for the sample of 82 Type 1 AGNs (82 rows)
4.J/MNRAS/472/334/table4The MIR parameters that we calculated and measured for the sample of 82 Type 1 AGNs (82 rows)
5.J/MNRAS/472/334/table5Flux measurements of the hydrogen recombination lines and obtained Balmer decrements for the Type 1 sample (74 rows)

Simple ConstraintList Of Constraints
 
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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+4)Name (char) NED name (meta.id;meta.main)
  (1)RAJ2000 deg (i) Right ascension (J2000) (pos.eq.ra;meta.main)
  (1)DEJ2000 deg (i) Declination (J2000) (pos.eq.dec;meta.main)
  (1+3)SDSS (char) SDSS name (JHHMMSS.ss+DDMMSS.ss) (meta.id)
  (1+5)PMF (char) SDSS plate-MJD-fiber (meta.id)
  (1+2)z  SDSS redshift (src.redshift)
  (1+2)Dist Mpc Angular size distance (pos.distance)
  (1+2)projdSDSS kpc Projected SDSS aperture diameter (phys.angSize;instr.fov)
  (1+2)projdirs kpc Projected IRS aperture diameter (phys.angSize;instr.fov)
  (1)Sp (char) Interactive spectrum from SDSS-DR14 (meta.ref.url)

ALL cols		    
 (i)indexed column
  (1+2)SimbadName (char) Designation understandable by the Simbad data-base (meta.id)
  (2)IRalpha  MIR spectral index from the literature (spect.index;em.IR.MIR)
  (2+4)RPAH  Fractional contributions of the PAH to the MIR luminosity from the literature (phys.luminosity;arith.ratio)
  (2+4)RAGN  Fractional contributions of the AGN to the MIR luminosity from the literature (phys.luminosity;arith.ratio)
  (2)log(OIII/Hb) [-] Line ratio [OIII]/Hβ from the literature (spect.line.intensity;arith.ratio)
  (2)log(NII/Ha) [-] Line ratio [NII]/Hα from the literature (spect.line.intensity;arith.ratio)
  (2)Refopt (char) Reference for the optical data (Note 1)   (meta.bib)
  (2)RefIR (char) Reference for the MIR (Note 1)   (meta.bib)
  (3)EWHbNLR 0.1nm NLR Hβ equivalent width (spect.line.eqWidth)
  (3)EWHbBROAD 0.1nm Broad Hβ equivalent width (EWHbBROAD = EWHbILR+EW(HbBLR) (spect.line.eqWidth)
  (3)EWFeII 0.1nm (n) FeII equivalent width (spect.line.eqWidth)
  (3)log(OIII/HbNLR) [-] (n) Line ratio [OIII]5007/HβNLR (spect.line.intensity;arith.ratio)
  (3)FWHMHb km/s Hβ FWHM (spect.line.width)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)log(L5100) [10-7W] log of luminosity of AGN at λ=5100Å, multiplied with 5100 (phys.luminosity;em.opt)
  (3)EWOIII 0.1nm Equivalent width for both components of doublet ([OIII]4959+[OIII]5007) (spect.line.eqWidth)
  (3)logNIIHaNLR [-] (n) Line ratio [NII]6583/HαNLR (spect.line.intensity;arith.ratio)
  (3)log(MBH) [Msun] log of black hole mass (phys.mass)
  (3)Fhost  Host fraction in the λλ4160-4210Å range, obtained in the decomposition (phys.luminosity;arith.ratio)
  (4)SSIL  Strength of a silicate feature (spect.line.width)
  (4)alpha  Spectralindex (spect.index)
  (4)L6 10-7W Monochromatic luminosity of the source at 6um (phys.luminosity;em.IR.4-8um)
  (4)L12 10-7W Monochromatic luminosity of the source at 12um (phys.luminosity;em.IR.8-15um)
  (4)EWPAH7.7 um (n) Equivalent width of PAH at 7.7um (spect.line.eqWidth;em.IR.4-8um)
  (4)EWPAH11.2 um (n) Equivalent width of PAH at 11.2um (spect.line.eqWidth;em.IR.8-15um)
  (4)R30/15  (n) Radio of fluxes at 30 and 15um (phot.flux;arith.ratio)
  (4)CVrmse  Coefficient of variation of the rms error (arith.rate)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)Chi2red  Reduced chi2 value (stat.fit.chi2)
  (5)HaNLR 10-20W/m2Hα NLR flux (phot.flux;em.line.Halpha;spect.line)
  (5)HbNLR 10-20W/m2Hβ NLR flux (phot.flux;em.line.Hbeta)
  (5)Habroad 10-20W/m2Hα broad flux (phot.flux;em.line.Halpha;spect.line)
  (5)Hbbroad 10-20W/m2Hβ broad flux (phot.flux;em.line.Hbeta)
  (5)NHa/Hb  Balmer decrement of the narrow lines (phot.flux;arith.ratio)
  (5)BHa/Hb  Balmer decrement of the broad lines (phot.flux;arith.ratio)

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