VizieR

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

  
VII/147
  Photometric Catalog of Northern Bright Galaxies (Kodaira+ 1992)
ReadMe+ftp
Similar Catalogs
Post annotation 		img(gal)
1.VII/147/data(c)The Catalog of Northern Bright Galaxies (791 rows)
2.VII/147/notesNotes on peculiar objects (72 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)
   (ALL)Name (char) The galaxy name taken from RSA (VII/51) (meta.id;meta.main)
  (1)RA1950 "h:m:s" (i) Hours of right ascension taken from RSA (VII/51) (Equinox 1950.0). (pos.eq.ra;meta.main)
  (1)DE1950 "d:m:s" (i) Degrees of declination (B1950) (pos.eq.dec;meta.main)
  (1)MType (char) Morphological type taken from RC2 and decoded by the authors. (src.morph.type)
  (1)TType  Morphological type index from RC2 (VII/112) (meta.code;src.morph.type)
  (1)u_TType (char) [:?] uncertainty/peculiarity code for TType (meta.note)
  (1)RVlg km/s Radial velocity relative to the centroid of the Local Group taken from RSA (VII/51) (spect.dopplerVeloc)
  (1)Av mag Galactic absorption in the V band calculated as AV = 0.75 AB, using the AB tabulated in Burstein and Heiles (1984ApJS...54...33B) (phys.absorption.gal;meta.modelled)
  (1)n_Av (char) Code for galactic absorption as in Burstein and Heiles (1984ApJS...54...33B). (meta.note)
  (1)Vmag mag Total apparent (asymptotic) magnitude in the V band derived in the growth curve fitting; estimated 1-sigma internal accuracy 0.10 mag. (phot.mag;em.opt.V)

ALL cols		    
 (i)indexed column
  (1)Reff [arcsec] Logarithm of the effective radius derived in the growth curve fitting; estimated internal accuracy 0.03. (phys.angSize)
  (1)u_Reff (char) Code for the effective radius (a colon shows values smaller than Re = 15 arcsec). (meta.code.error)
  (1)Gcurve (char) Category of growth curve template used (Note 2)   (phot.mag;meta.modelled)
  (1)Vmag25 mag Apparent magnitude integrated in the 25mag/arcsec2 isophote (Note 3)   (phot.mag;em.opt.V)
  (1)a [arcsec] Logarithm of semi-major axis of the envelope ellipse; estimated internal accuracy 0.03. (phys.angSize)
  (1)b/a  Axis ratio of the envelope ellipse; estimated internal accuracy 0.04. (phys.angSize;arith.ratio)
  (1)ePA deg Angle of the envelope ellipse (Note 1)   (pos.posAng)
  (1)fPA deg Position angle of the frame (Note 1)   (pos.posAng)
  (1)mu mag/arcsec2Effective surface brightness (Note 5)   (phot.mag.sb;em.opt.V)
  (1)u_mu (char) Uncertainty code for mu (Note 5)   (meta.code.error)
  (1)Aeff [arcsec] Logarithm of the semi-major axis of effective ellipse (Note 5)   (phys.angSize.smajAxis)
  (1)u_Aeff (char) Uncertainty code for Aeff (Note 5)   (meta.code.error)
  (1)B/A  The axis ratio of the effective ellipse; the estimated internal accuracy is 0.03. (phys.angSize)

ALL cols		    
 (i)indexed column
  (1)c1  The luminosity concentration index 1/4,3/4 (Note 4)   (phys.size;arith.ratio)
  (1)u_c1 (char) Uncertainty code for c1 (Note 4)   (meta.code.error)
  (1)c2  The luminosity concentration index 1/2,3/4 (Note 4)   (phys.size;arith.ratio)
  (1)u_c2 (char) Uncertainty code for c2 (Note 4)   (meta.code.error)
  (1)Note (char) [N] indicates that a note is given on the galaxy at the end of the catalog (Kodaira et al. 1990). (meta.note)
  (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)_RA.icrs "h:m:s" (n)(i) Right ascension (ICRS) (computed by VizieR, not part of the original data) (pos.eq.ra)
  (1)_DE.icrs "d:m:s" (n)(i) Declination (ICRS) (computed by VizieR, not part of the original data) (pos.eq.dec)
  (2)Text (char) Text of note (meta.note)

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