VizieR

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

VizieR

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J/AJ/144/11
  IR imaging, nuclear SEDs & Spitzer spectra of 22 AGNs (Mason+, 2012)
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2012AJ....144...11M
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spectrum/SED
Post annotation 		img(gal)
1.J/AJ/144/11/galaxies(c)Properties of the low-luminosity active galactic nuclei (LLAGNs) (tables 1 and 5 of paper) (22 rows)
2.J/AJ/144/11/photoPhotometric results (near- and mid-IR) (tables 3 and 4 of paper) (43 rows)
3.J/AJ/144/11/table6Intrinsic X-Ray luminosity estimates for suspected Compton-thick low-luminosity active galactic nuclei (LLAGNs) (6 rows)
4.J/AJ/144/11/table7Spectral energy distribution data (446 rows)
5.J/AJ/144/11/refsReferences (110 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+3+4)NGC  (i) NGC galaxy number (meta.id;meta.main)
  (1)OName (char) Other galaxy name (meta.id)
  (1)MType (char) Morphological type (src.morph.type)
  (1)AGNt (char) AGN type (LL=low-luminosity, S=Seyfert) (src.class)
  (1)Dist Mpc (n) Distance (pos.distance;pos.heliocentric)
  (1)logMBH [Msun] (n) [7.1/9] log of black hole mass (phys.mass)
  (1)logER  (n) log of the Eddington ratio Lbol/LEdd (phys.luminosity;arith.ratio)
  (1)Rx [-] (n) [-5.3/-1.1] Radio to X emission ratio RX (Note 1)   (phys.luminosity;arith.ratio)
  (1)Cat  (n)Category depending on the Eddington ratio and radio emission (Note 3)   (src.class)
  (1)SMBH (char) Evidence that the galaxy hosts an actively accreting supermassive black hole (SMBH), with reference. See Section 2 for more details (Note 2)   (meta.code)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)SED (char) SED plot(from table7) (meta.ref.url)
  (1)Simbad (char) ask the Simbad data-base about this object (meta.ref)
  (1)NED (char) ask the NED data-base about this object (meta.ref)
  (1)Fpsf/F2  (n) Ratio of mid-IR PSF-scaling flux to that obtained in a 2" aperture (see Section 3.1 for details) (Note 4)   (phot.flux;arith.ratio)
  (1)S  (n) Strength of the ∼10µm silicate feature S10 (see Section 4.2 for details) (Note 5)   (spect.line.intensity)
  (1)alpha  (n) Near- to mid-IR spectral index αIR, F(ν)∝ν–α, for objects possessing at least one mid-IR and one H-band photometric point. See Section 4.3 (Note 4)   (spect.index)
  (1)l_logLMIR (char) Upper limit on log(LMIR) (meta.code.error)
  (1)logLMIR [10-7W] [39.8/42.7] log of mid-infrared luminosity (Note 4)   (phys.luminosity;em.IR)
  (1)logLX [10-7W] [38.8/41.4] absorption-corrected 2-10keV X-ray luminosity (erg/s); see Section 4.3 (phys.luminosity;em.X-ray)
  (1)r_logLX  Reference for logLX (X-ray luminosity) and for NH (HI column density), in refs. dat file (meta.ref;pos.frame)
  (1)l_NH (char) Upper limit on NH (meta.code.error)
  (1)NH 10+22cm-2(n) HI column density (phys.columnDensity)
  (1)CT (char) Indicates whether the galaxy is suspected to be Compton-thick (Y, N or ?) (Note 6)   (meta.code)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)r_CT  (n) Reference for CT, in refs.dat file (meta.ref;pos.frame)
  (1)_RA deg (i) Positions from SIMBAD database (right ascension part) (pos.eq.ra;meta.main)
  (1)_DE deg (i) Positions from SIMBAD database (declination part) (pos.eq.dec;meta.main)
  (2)f_NGC (char) Flag on NGC (Note 1)   (meta.code)
  (2)Flt (char) Filter used (Note 4)   (instr.setup;instr.filter)
  (2)l_F2 (char) Upper limit on F2 (meta.code.error)
  (2)F2 mJy [3/257] Photometric flux in 2" diameter aperture (phot.flux.density;instr.fov)
  (2)e_F2 mJy (n) Error in F2 (stat.error)
  (2)Fpsf mJy (n) [2/197] PSF-scaling photometry (Note 2)   (phot.flux)
  (2)f_Fpsf (char) [e] Questionable Fpsf (Note 3)   (meta.code)
  (2)e_Fpsf mJy (n) Error in Fpsf (stat.error)
  (2)FWHMg arcsec (n) FWHM (Moffat) of galactic nucleus (phys.angSize)
  (2)f_FWHMg (char) [f] Gaussian FWHMg (Note 3)   (meta.code)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)FWHMs arcsec FWHM (Moffat) of standard star (phys.angSize)
  (2)f_FWHMs (char) [f] Gaussian FWHMs (Note 3)   (meta.code)
  (3)logLX 10-7W [39/41.1] Intrinsic luminosity estimates as given in Table 5 (Column logLX), from spectral fitting of high-resolution X-ray data (Note 1)   (phys.luminosity;em.X-ray)
  (3)logLX([OIII]) 10-7W [40.6/42.9] Intrinsic "corrected" luminosity from Gonzalez-Martin et al. (2009A&A...506.1107G) and Panessa et al. (2006A&A...455..173P) (Note 2)   (phys.luminosity;em.X-ray)
  (3)logLX([OIV]) 10-7W (n) [39.3/41.6] Intrinsic luminosity estimates based on Lbol,AGN-L[OIV] relation of Goulding et al. (2010MNRAS.406..597G) (Note 3)   (phys.luminosity;em.X-ray)
  (4)nu Hz Frequency of observation ν (em.freq;obs)
  (4)l_Lum (char) Limit flag on Lum (meta.code.error)
  (4)Lum 10-7W The νLν luminosity; in erg/s (phys.luminosity)
  (4)Aper (char) arcsec Aperture/resolution (Note 1)   (phys.angSize)
  (4)Facility (char) Telescope/instrument (meta.note)
  (4)Ref (char) Reference(s), in refs.dat file (meta.ref;pos.frame;meta.file)
  (5)Ref   [1/110] Reference number (meta.id;meta.main)
  (5)BibCode (char) Bibliographic code (meta.bib.bibcode)
  (5)Aut (char) Author's name (meta.bib.author)
  (5)Com (char) Comments (meta.note)

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