Complement to VIII/85A

Source WB_1601-0021: 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 J1603.8-0029                 5.94e+03  1.2e+03      79.98   68864 0   -0.72    5.12  240.9704  -00.4965
   80  Cula 1601-003                     7.00e+03  1.4e+03     222.00   68864 0   -0.72    5.12  240.9787  -00.5078
  160  Culb 1601-003                     4.80e+03  9.6e+02     111.00   68864 0   -0.72    5.12  240.9787  -00.5078
  365  TXS 1601-003                      1.79e+03  3.6e+02       6.00   68864 0   -0.72    5.12  240.9715  -00.4979
  408  MRC 1601-003                      1.66e+03  3.3e+02     120.00   68864 0   -0.72    5.12  240.9712  -00.4961
 1400  FIRST J160353.1-002953            6.67e+02  1.3e+02       5.00   68864 0   -0.72    5.12  240.9714  -00.4981
 1400  NVSS J160353-002952               7.16e+02  1.4e+02      45.00   68864 0   -0.72    5.12  240.9711  -00.4978
 1400  WB 1601-0021                      7.19e+02  1.4e+02     120.00   68864 0   -0.69    5.01  240.9696  -00.4894
 2700  PKS J1603-0029                    4.50e+02  9.0e+01      60.00   68864 0   -0.72    5.12  240.9712  -00.4981
 4850  BWE 1601-0021                     3.04e+02  6.1e+01     138.00   68864 0   -0.69    5.01  240.9696  -00.4894
 4850  MITG J160351-0030                 2.75e+02  5.5e+01     258.00   68864 0   -0.73    5.15  240.9663  -00.5017
 4850  PMN J1603-0029                    3.26e+02  6.5e+01     168.00   68864 0   -0.73    5.15  240.9762  -00.4992

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  


   408  MRC 1601-003                      1.66e+03  3.3e+02     120.00    68864  240.9712  -00.4961
  1400  FIRST J160349.8-002933            7.50e+00  1.5e+00       5.00   -68864  240.9577  -00.4927
  4850  MITG J160351-0030                 2.75e+02  5.5e+01     258.00    68864  240.9663  -00.5017
  4850  PMN J1603-0029                    3.26e+02  6.5e+01     168.00    68864  240.9762  -00.4992

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