Complement to VIII/85A

Source 6C_092606+463510: 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  


  151  6C 092606+463510                  4.40e+02  8.8e+01     252.00   39781 0   -0.69    4.14  142.3479  +46.3669
  151  7C 092605.90+463356.00            3.45e+02  6.9e+01      70.20   39781 0   -0.57    3.78  142.3458  +46.3464
  232  MY 092608.7+462048.1              3.50e+02  7.0e+01     150.00   39781 0   -0.55    3.71  142.3575  +46.3467
  325  WN B0926.0+4633                   1.96e+02  3.9e+01      12.00   39781 0   -0.57    3.78  142.3434  +46.3458
  408  B3 0926+465                       1.80e+02  3.6e+01      84.00   39781 0   -0.57    3.78  142.3417  +46.3569
 1400  FIRST J092922.6+462046            6.31e+01  1.3e+01       5.00   39781 0   -0.65    3.96  142.3445  +46.3462
 1400  NVSS J092922+462046               9.50e+01  1.9e+01      45.00   39781 0   -0.58    3.80  142.3446  +46.3462
 1400  WB 0926+4633                      1.17e+02  2.3e+01     120.00   39781 0   -0.64    4.04  142.3467  +46.3419
 4850  87GB 092606.1+463343              4.80e+01  9.6e+00     138.00   39781 0   -0.67    4.09  142.3467  +46.3428
 4850  BWE 0926+4633                     4.60e+01  9.2e+00     138.00   39781 0   -0.65    4.06  142.3467  +46.3419
 4850  GB6 B0926+4634                    5.00e+01  1.0e+01     108.00   39781 0   -0.69    4.14  142.3479  +46.3483

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  


   151  7C 092605.90+463356.00            3.45e+02  6.9e+01      70.20    39781  142.3458  +46.3464
   232  MY 092608.7+462048.1              3.50e+02  7.0e+01     150.00    39781  142.3575  +46.3467
   325  WN B0926.0+4633                   1.96e+02  3.9e+01      12.00    39781  142.3434  +46.3458
  1400  FIRST J092924.7+462053            9.00e+00  1.8e+00       5.00   -39781  142.3529  +46.3482
  4850  87GB 092606.1+463343              4.80e+01  9.6e+00     138.00    39781  142.3467  +46.3428

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