Complement to VIII/85A

Source BWE_0249+1706: 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  


  365  TXS 0249+171                      4.20e+02  8.4e+01       6.00    9137 0   -0.24    3.25  043.0318  +17.3119
 1400  NVSS J025207+171843               2.40e+02  4.8e+01      45.00    9137 0   -0.24    3.25  043.0320  +17.3120
 1400  WB 0249+1706                      2.40e+02  4.8e+01     120.00    9137 0   -0.24    3.25  043.0337  +17.3117
 4850  87GB 024920.2+170623              2.32e+02  4.6e+01     138.00    9137 0   -0.24    3.25  043.0333  +17.3111
 4850  BWE 0249+1706                     1.97e+02  3.9e+01     138.00    9137 0   -0.29    3.37  043.0337  +17.3117
 4850  GB6 B0249+1706                    2.36e+02  4.7e+01     108.00    9137 0   -0.24    3.25  043.0329  +17.3117
 4850  MITG J025210+1718                 2.31e+02  4.6e+01     258.00    9137 0   -0.24    3.25  043.0417  +17.3089
 4850  MITG J025213+1718                 1.39e+02  2.8e+01     258.00    9137 0   -0.43    3.72  043.0554  +17.3042
 8400  CLASS J025207.7192+171842.685     1.95e+02  3.9e+01       0.33    9137 0   -0.24    3.25  043.0321  +17.3119
 8400  JVAS J0252+1718                   1.95e+02  3.9e+01       0.33    9137 0   -0.24    3.25  043.0322  +17.3119

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 J0252.1+1718                 1.49e+03  3.0e+02      79.98    -9137  043.0312  +17.3127
   365  TXS 0249+171                      4.20e+02  8.4e+01       6.00     9137  043.0318  +17.3119
  1400  WB 0249+1706                      2.40e+02  4.8e+01     120.00     9137  043.0337  +17.3117
  4850  87GB 024920.2+170623              2.32e+02  4.6e+01     138.00     9137  043.0333  +17.3111
  4850  MITG J025213+1718                 1.39e+02  2.8e+01     258.00     9137  043.0554  +17.3042
  8400  CLASS J025207.7192+171842.685     1.95e+02  3.9e+01       0.33     9137  043.0321  +17.3119

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