Complement to VIII/85A

Source Culb_0322-035: points from spectra and waste tables

  Postscript Figure Additional frequencies and fluxes in ν and S Data as a Table  
Adapt
Plot
nu
S
x cuts: xlog Bitmap size:
y cuts: ylog 
"-c="

The 2 columns in color are computed by VizieR, and are not part of the original data.
The column SED is a link to a plot of the radio spectrum, and the column Radio+Opt is a link to an Aladin preview. The SED plot contains points from the cross-identification (spectra; red), from the waste basket (waste; yellow), and the fitted radio spectra as lines. The Aladin preview contains a DSS image together with NVSS contours (blue) and the points and associated beams of the radio spectrum (red); points and beams of the sources from the waste basket are hidden but can be made visible by clicking on the corresponding plane (yellow).
VIII/85A/spectra
Post annotation 		SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009) [ReadMe+ftp]
2010A&A...511A..53V

The parameters of the radio spectra[image][spectrum] (631736 rows)		img(gal)
start AladinLite 
  nu   Name                               S(nu)       e        beam      Seq  n     a       b     RAJ2000   DEJ2000
 MHz                                       mJy       mJy      arcsec                      [mJy]     deg       deg  


   74  VLSS J0324.6-0324                 1.02e+04  2.0e+03      79.98   12173 5   -0.88    5.76  051.1708  -03.4055
   80  Cula 0322-035                     1.30e+04  2.6e+03     222.00   12173 5   -0.90    5.82  051.1754  -03.4147
  160  Culb 0322-035                     6.60e+03  1.3e+03     111.00   12173 5   -0.94    5.97  051.1754  -03.4147
  178  4C -03.12                         7.10e+03  2.1e+03     690.00   12173 5   -0.94    5.97  051.1763  -03.4500
  365  TXS 0322-035                      4.74e+03  9.5e+02       6.00   12173 5   -0.94    5.97  051.1752  -03.4130
  408  MRC 0322-035                      4.04e+03  8.1e+02     120.00   12173 5   -0.94    5.97  051.1767  -03.4133
 1400  NVSS J032441-032419               6.86e+02  1.4e+02      45.00   12173 5   -0.80    5.38  051.1717  -03.4055
 1400  WB 0322-0335                      1.19e+03  2.4e+02     120.00   12173 5   -0.94    5.97  051.1717  -03.4114
 2700  PKS J0324-0324                    5.50e+02  1.1e+02      60.00   12173 5   -0.94    5.97  051.1792  -03.4117
 4850  PMN J0324-0325                    2.73e+02  5.5e+01     168.00   12173 5   -0.94    5.97  051.1725  -03.4175

The column SED is a link to a plot of the radio spectrum, and the column Radio+Opt is a link to an Aladin preview. The SED plot contains points from the cross-identification (spectra; red), from the waste basket (waste; yellow), and the fitted radio spectra as lines. The Aladin preview contains a DSS image together with NVSS contours (blue) and the points and associated beams of the radio spectrum (red); points and beams of the sources from the waste basket are hidden but can be made visible by clicking on the corresponding plane (yellow).
VIII/85A/waste
Post annotation 		SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009) [ReadMe+ftp]
2010A&A...511A..53V

Source parameters based on positional cross-id[spectrum] (1497216 rows)		img(gal)
start AladinLite 
  nu    Name                               S(nu)       e        beam      Seq     RAJ2000   DEJ2000
  MHz                                       mJy       mJy      arcsec               deg       deg  


    74  VLSS J0324.7-0325                 6.85e+03  1.4e+03      79.98   -12173  051.1829  -03.4282
   160  Culb 0322-035                     6.60e+03  1.3e+03     111.00    12173  051.1754  -03.4147
   178  4C -03.12                         7.10e+03  2.1e+03     690.00    12173  051.1763  -03.4500
   408  MRC 0322-035                      4.04e+03  8.1e+02     120.00    12173  051.1767  -03.4133
  1400  NVSS J032444-032543               4.15e+02  8.3e+01      45.00   -12173  051.1838  -03.4288
  4850  PMN J0324-0325                    2.73e+02  5.5e+01     168.00    12173  051.1725  -03.4175

Note: For the spectrum finding algorithm, the errors have been increased by 50%