Complement to VIII/85A

Source GB6_B1252+4112: 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 J1254.3+4055                 6.90e+02  1.4e+02      79.98   51606 0   -0.73    4.20  193.5971  +40.9331
  151  6C 125203+411222                  3.10e+02  6.2e+01     252.00   51606 0   -0.65    3.90  193.6004  +40.9353
  151  7C 125204.40+411214.00            4.01e+02  8.0e+01      70.20   51606 0   -0.73    4.20  193.6029  +40.9331
  232  MY 125205.2+405521.4              2.00e+02  4.6e+01     150.00   51606 0   -0.65    3.90  193.6067  +40.9226
  325  WN B1252.0+4112                   2.21e+02  4.4e+01      12.00   51606 0   -0.70    4.11  193.6019  +40.9323
  408  B3 1252+412                       2.10e+02  4.2e+01      84.00   51606 0   -0.73    4.20  193.5992  +40.9347
 1400  FIRST J125424.6+405555            4.92e+01  9.8e+00       5.00   51606 0   -0.49    3.32  193.6029  +40.9321
 1400  NVSS J125424+405556               7.27e+01  1.5e+01      45.00   51606 0   -0.70    4.11  193.6019  +40.9323
 4850  BWE 1252+4112                     3.30e+01  6.8e+00     138.00   51606 0   -0.65    3.90  193.5975  +40.9347
 4850  GB6 B1252+4112                    3.30e+01  6.6e+00     108.00   51606 0   -0.65    3.90  193.5925  +40.9333

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 J1254.3+4055                 6.90e+02  1.4e+02      79.98    51606  193.5971  +40.9331
   151  6C 125203+411222                  3.10e+02  6.2e+01     252.00    51606  193.6004  +40.9353
   232  MY 125205.2+405521.4              2.00e+02  4.6e+01     150.00    51606  193.6067  +40.9226
   408  B3 1252+412                       2.10e+02  4.2e+01      84.00    51606  193.5992  +40.9347
  1400  FIRST J125424.3+405601            1.79e+01  3.6e+00       5.00   -51606  193.6013  +40.9336
  4850  GB6 B1252+4112                    3.30e+01  6.6e+00     108.00    51606  193.5925  +40.9333

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