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:
 Target dimension:
NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/MNRAS/489/3351
  Spectral energy distributions of AGNs (Brown+, 2019)
ReadMe+ftp
2019MNRAS.489.3351B
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spectrum
Post annotation 		img(gal)
1.J/MNRAS/489/3351/table1(c)The basic properties of the sample and the SED wavelength ranges[spectrum] (41 rows)
2.J/MNRAS/489/3351/table2The sources of spectroscopy used for the SEDs (41 rows)
3.J/MNRAS/489/3351/tablea1(c)Measured photometry (in mJy) corrected for Milky Way foreground extinction (41 rows)
4.J/MNRAS/489/3351/tablea2(c)Synthetic photometry (in mJy) derived from the SEDs (41 rows)

Simple ConstraintList Of Constraints
 
Query by Constraints constraints help applied on Columns (Output Order: + - )
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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)
   (ALL)Name (char) Galaxy name (meta.id;meta.main)
  (1+3+4)RAJ2000 deg (i) Right ascension (J2000) (pos.eq.ra;meta.main)
  (1+3+4)DEJ2000 deg (i) Declination (J2000) (pos.eq.dec;meta.main)
  (1)z  Redshift (src.redshift)
  (1)gmag mag g-band magnitude (phot.mag;em.opt.B)
  (1)gMAG mag g-band absolute magnitude (phys.magAbs)
  (1)E(B-V) mag E(B-V) colour excess (phot.color.excess)
  (1)Aper arcsec Photometric aperture (phys.angSize;instr.fov)
  (1)Class (char) AGN class from Veron-Cetty & Veron (2010A&A...518A..10V, Cat. VII/258) (src.class)
  (1)EW 0.1nm (n) Equivalent width (H{alpha}+[NII]) (spect.line.eqWidth)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)lambdamin um SED wavelenght range {lambda}min (instr.bandwidth)
  (1)lambdamax um SED wavelenght range {lambda}max (instr.bandwidth)
  (1)scalemin  Scaling minimum value (Note 1)   (instr.scale)
  (1)scalemax  Scaling maximum value (Note 1)   (instr.scale)
  (1)SED (char) Spectral energy distribution (meta.ref.url)
  (1)SimbadName (char) (n)Designation understandable by the Simbad data-base (meta.id)
  (2)rinf0.01 (char) Source of the <0.01µm spectra (Note 1)   (meta.bib)
  (2)r0.09-0.33 (char) Source of the 0.09-0.33µm spectra (Note 1)   (meta.bib)
  (2)r0.33-1.0 (char) Source of the 0.33-1.0µm spectra (Note 1)   (meta.bib)
  (2)r1.0-2.5 (char) Source of the 1.0-2.5µm spectra (Note 1)   (meta.bib)
  (2)r2.5-5 (char) Source of the 2.5-5µm spectra (Note 1)   (meta.bib)
  (2)r5-42 (char) Source of the 5-42µm spectra (Note 1)   (meta.bib)
  (2)r42-500 (char) Source of the 42-500µm spectra (Note 1)   (meta.bib)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3+4)FFUV mJy (n) FUV flux from GALEX (phot.flux;em.UV)
  (3+4)FUVW2 mJy (n) UVW2 flux from Swift/UVOT (phot.flux;em.UV)
  (3+4)FUVM2 mJy (n) UVM2 flux from Swift/UVOT (phot.flux;em.UV)
  (3+4)FNUV mJy (n) NUV flux from GALEX (phot.flux;em.UV)
  (3+4)FUVW1 mJy (n) UVW1 flux from Swift/UVOT (phot.flux;em.UV)
  (3+4)FUSwift mJy (n) Flux on the Swift/UVOT U-band (phot.flux.density;em.opt.U)
  (3+4)FuSM mJy (n) Flux on the SkyMapper u-band (phot.flux.density;em.opt.U)
  (3+4)FuSDSS mJy (n) Flux on the SDSS u-band (phot.mag;em.opt.U)
  (3+4)FvSM mJy (n) Flux on the SkyMapper v-band (phot.flux.density;em.opt.V)
  (3+4)FBSwift mJy (n) Flux on the Swift/UVOT B-band (phot.flux.density;em.opt.B)
  (3+4)FgSDSS mJy (n) Flux on the SDSS g-band (phot.mag;em.opt.B)
  (3+4)FgPS1 mJy (n) Flux on the Pan-STARRS1 g-band (phot.mag;em.opt.B)
  (3+4)FgSM mJy (n) Flux on the SkyMapper g-band (phot.mag;em.opt.B)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3+4)FVSwift mJy (n) Flux on the Swift/UVOT V-band (phot.flux.density;em.opt.V)
  (3+4)FrSDSS mJy (n) Flux on the SDSS r-band (phot.mag;em.opt.R)
  (3+4)FrPS1 mJy (n) Flux on the Pan-STARRS1 r-band (phot.mag;em.opt.R)
  (3+4)FrSM mJy (n) Flux on the SkyMapper r-band (phot.mag;em.opt.R)
  (3+4)FiSDSS mJy (n) Flux on the SDSS i-band (phot.mag;em.opt.I)
  (3+4)FiPS1 mJy (n) Flux on the Pan-STARRS1 i-band (phot.mag;em.opt.I)
  (3+4)FiSM mJy (n) Flux on the SkyMapper i-band (phot.mag;em.opt.I)
  (3+4)FzPS1 mJy (n) Flux on the Pan-STARRS1 i-band (phot.mag;em.opt.I)
  (3+4)FzSDSS mJy (n) Flux on the SDSS z-band (phot.mag;em.opt.I)
  (3+4)FzSM mJy (n) Flux on the SkyMapper z-band (phot.mag;em.opt.I)
  (3+4)FyPS1 mJy (n) Flux on the Pan-STARRS1 y-band (phot.flux.density;em.IR.J)
  (3+4)FJ mJy Flux on the 2MASS J-band (phot.flux.density;em.IR.J)
  (3+4)FH mJy Flux on the 2MASS H-band (phot.flux.density;em.IR.H)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3+4)FK mJy Flux on the 2MASS K-band (phot.mag;em.IR.K)
  (3+4)FW1 mJy Flux on the WISE W1 band (phot.mag;em.IR.3-4um)
  (3+4)F3.6 mJy (n) Sptizer/IRAC 3.6um flux (phot.mag;em.IR.3-4um)
  (3+4)F4.5 mJy (n) Sptizer/IRAC 4.5um flux (phot.mag;em.IR.4-8um)
  (3+4)FW2 mJy Flux on the WISE W2 band (phot.mag;em.IR.4-8um)
  (3+4)F5.8 mJy (n) Sptizer/IRAC 5.8um flux (phot.mag;em.IR.4-8um)
  (3+4)F8.0 mJy (n) Sptizer/IRAC 8.0um flux (phot.flux.density;em.IR.8-15um)
  (3+4)FW3 mJy Flux on the WISE W3 band (phot.flux.density;em.IR.8-15um)
  (3+4)FW4 mJy Flux on the WISE W4 band (phot.flux.density;em.IR.15-30um)
  (3+4)F24 mJy (n) Spitzer/MIPS 24um flux (phot.flux.density;em.IR.15-30um)
  (3+4)F70 mJy (n) Herschel/PACS 70um flux (phot.flux.density;em.IR.30-60um)
  (3+4)F100 mJy (n) Herschel/PACS 100um flux (phot.flux.density;em.IR.60-100um)
  (3+4)F160 mJy (n) Herschel/PACS 160um flux (phot.flux.density;em.mm.1500-3000GHz)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3+4)F250 mJy (n) Herschel/SPIRE 250um flux (phot.flux.density;em.mm.750-1500GHz)
  (3+4)F350 mJy (n) Herschel/SPIRE 350um flux (phot.flux.density;em.mm.750-1500GHz)
  (3+4)F500 mJy (n) Herschel/SPIRE 500um flux (phot.flux.density;em.mm.400-750GHz)

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