Complement to VIII/85A

Source GB6_B0059+4158: 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  


  325  WN B0059.6+4158                   3.90e+01  7.8e+00      12.00    2244 0    0.37    0.67  015.6132  +42.2394
 4850  87GB 005937.6+415801              1.36e+02  2.7e+01     138.00    2244 0    0.37    0.67  015.6137  +42.2356
 4850  BWE 0059+4158                     1.33e+02  2.7e+01     138.00    2244 0    0.37    0.67  015.6146  +42.2361
 4850  GB6 B0059+4158                    1.21e+02  2.4e+01     108.00    2244 0    0.37    0.67  015.6137  +42.2372
 8400  CLASS J010227.1533+421418.993     1.29e+02  2.6e+01       0.33    2244 0    0.37    0.67  015.6131  +42.2386

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  


   325  WN B0059.6+4158                   3.90e+01  7.8e+00      12.00     2244  015.6132  +42.2394
  1400  NVSS J010227+421418               4.23e+01  8.5e+00      45.00    -2244  015.6135  +42.2386
  4850  87GB 005937.6+415801              1.36e+02  2.7e+01     138.00     2244  015.6137  +42.2356
  4850  BWE 0059+4158                     1.33e+02  2.7e+01     138.00     2244  015.6146  +42.2361
  4850  GB6 B0059+4158                    1.21e+02  2.4e+01     108.00     2244  015.6137  +42.2372
  8400  CLASS J010224.0676+421419.748     6.60e+00  1.3e+00       0.33    -2244  015.6003  +42.2388
  8400  CLASS J010225.2658+421419.446     7.40e+00  1.5e+00       0.33    -2244  015.6052  +42.2387
  8400  CLASS J010225.5975+421434.100     4.80e+00  1.0e+00       0.33    -2244  015.6066  +42.2428
  8400  CLASS J010227.1533+421418.993     1.29e+02  2.6e+01       0.33     2244  015.6131  +42.2386
  8400  CLASS J010227.4387+421423.649     2.40e+00  5.0e-01       0.33    -2244  015.6143  +42.2399
  8400  CLASS J010228.4493+421423.457     3.90e+00  8.0e-01       0.33    -2244  015.6185  +42.2398
  8400  CLASS J010228.5635+421418.664     1.40e+00  3.0e-01       0.33    -2244  015.6190  +42.2385

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