Complement to VIII/85A

Source 4C_+50.54: 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 J2113.5+5039                 5.18e+03  1.0e+03      79.98   87506 0   -0.69    5.11  318.3796  +50.6531
  178  4C +50.54                         3.20e+03  9.6e+02     690.00   87506 0   -0.67    5.06  318.3808  +50.6350
  232  MY 211151.9+503905.7              3.04e+03  6.1e+02     150.00   87506 0   -0.69    5.11  318.3813  +50.6516
  325  WN B2111.8+5026                   2.97e+03  5.9e+02      12.00   87506 0   -0.69    5.11  318.3806  +50.6532
  327  WSRTGP 2111+5026                  2.36e+03  4.7e+02      60.00   87506 0   -0.69    5.11  318.3811  +50.6533
  365  TXS 2111+504                      3.02e+03  6.0e+02       6.00   87506 0   -0.69    5.11  318.3816  +50.6532
 1400  NVSS J211331+503912               8.86e+02  1.8e+02      45.00   87506 0   -0.69    5.11  318.3810  +50.6534
 1410  RRF 844                           1.17e+03  2.3e+02     564.00   87506 0   -0.67    5.06  318.4129  +50.6758
 2700  F3R 2946                          5.40e+02  1.1e+02     150.00   87506 0   -0.69    5.11  318.3883  +50.6508
 4850  87GB 211152.0+502656              2.93e+02  5.9e+01     138.00   87506 0   -0.70    5.15  318.3821  +50.6564
 4850  BWE 2111+5026                     2.49e+02  5.0e+01     138.00   87506 0   -0.97    5.97  318.3825  +50.6564
 4850  GB6 B2111+5026                    2.67e+02  5.3e+01     108.00   87506 0   -0.92    5.84  318.3808  +50.6544

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  


   178  4C +50.54                         3.20e+03  9.6e+02     690.00    87506  318.3808  +50.6350
  1400  NVSS J211334+503639               4.90e+00  1.0e+00      45.00   -87506  318.3956  +50.6109
  1400  NVSS J211344+503904               2.90e+00  6.0e-01      45.00   -87506  318.4336  +50.6511
  1410  RRF 844                           1.17e+03  2.3e+02     564.00    87506  318.4129  +50.6758

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