Complement to VIII/85A

Source MRC_0047-103: 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 J0049.8-1006                 3.14e+03  6.3e+02      79.98    4680 0   -0.48    4.42  012.4750  -10.1048
   80  Cula 0047-103                     3.00e+03  6.0e+02     222.00    4680 0   -0.58    4.65  012.4800  -10.0967
  160  Culb 0047-103                     2.30e+03  4.6e+02     111.00    4680 0   -0.46    4.35  012.4800  -10.0967
  365  TXS 0047-103                      1.88e+03  3.8e+02       6.00    4680 0   -0.48    4.42  012.4756  -10.1039
  408  MRC 0047-103                      1.77e+03  3.5e+02     120.00    4680 0   -0.58    4.64  012.4771  -10.1050
 1400  FIRST J004954.1-100614            8.15e+02  1.6e+02       5.00    4680 0   -0.48    4.42  012.4754  -10.1041
 1400  NVSS J004954-100614               8.25e+02  1.7e+02      45.00    4680 0   -0.47    4.40  012.4754  -10.1040
 2700  PKS J0049-1006                    5.80e+02  1.2e+02      60.00    4680 0   -0.47    4.40  012.4725  -10.1056
 4850  PMN J0049-1006                    3.17e+02  6.3e+01     168.00    4680 0   -0.58    4.64  012.4787  -10.1058

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 J0049.8-1006                 3.14e+03  6.3e+02      79.98     4680  012.4750  -10.1048
   160  Culb 0047-103                     2.30e+03  4.6e+02     111.00     4680  012.4800  -10.0967
   408  MRC 0047-103                      1.77e+03  3.5e+02     120.00     4680  012.4771  -10.1050
  1400  FIRST J004954.9-100635            8.00e-01  2.0e-01       5.00    -4680  012.4789  -10.1098
  1400  FIRST J004956.0-100708            9.00e-01  2.0e-01       5.00    -4680  012.4837  -10.1190
  2700  PKS J0049-1006                    5.80e+02  1.2e+02      60.00     4680  012.4725  -10.1056
  4850  PMN J0049-1006                    3.17e+02  6.3e+01     168.00     4680  012.4787  -10.1058

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