Complement to VIII/85A

Source GB6_B0050+4017: 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 J0053.5+4034                 1.45e+03  2.9e+02      79.98    1934 5   -0.78    4.66  013.3827  +40.5781
  151  7C 005045.70+401822.00            9.21e+02  1.8e+02      70.20    1934 5   -0.78    4.66  013.3845  +40.5772
  232  MY 005048.5+403446.6              6.70e+02  1.3e+02     150.00    1934 5   -0.76    4.63  013.3963  +40.5796
  325  WN B0050.7+4018                   5.28e+02  1.1e+02      12.00    1934 5   -0.78    4.66  013.3840  +40.5751
  325  WN B0050.7+4018B                  3.79e+02  7.6e+01      12.00    1934 5   -0.78    4.66  013.3854  +40.5799
  408  B3 0050+403                       4.20e+02  8.4e+01      84.00    1934 5   -0.78    4.66  013.3863  +40.5778
 1400  NVSS J005332+403443               1.10e+02  2.2e+01      45.00    1934 5   -0.78    4.66  013.3848  +40.5788
 4730  B3a 0050+403                      6.00e+01  1.2e+01     168.00    1934 5   -0.77    4.59  013.3859  +40.5780
 4850  87GB 005043.8+401741              6.21e+01  1.2e+01     138.00    1934 5   -0.77    4.59  013.3767  +40.5658
 4850  BWE 0050+4017                     6.50e+01  1.3e+01     138.00    1934 5   -0.77    4.59  013.3792  +40.5661
 4850  GB6 B0050+4017                    5.44e+01  1.1e+01     108.00    1934 5   -0.78    4.66  013.3796  +40.5656

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  


   159  3C 24                             9.50e+03  1.9e+03     600.00    -1934  013.3562  +40.4717
   325  WN B0050.7+4018A                  1.48e+02  3.0e+01      12.00    -1934  013.3802  +40.5612
  1400  NVSS J005322+403258               2.70e+00  5.0e-01      45.00    -1934  013.3429  +40.5495
  1400  NVSS J005331+403327               4.72e+01  9.4e+00      45.00    -1934  013.3819  +40.5575
  4850  87GB 005043.8+401741              6.21e+01  1.2e+01     138.00     1934  013.3767  +40.5658

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