Complement to VIII/85A

Source TXS_1641+320: 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 J1643.1+3156                 9.60e+02  1.9e+02      79.98   72764 0   -0.65    4.21  250.7979  +31.9392
  151  6C 164119+320125                  7.70e+02  1.5e+02     252.00   72764 0   -0.62    4.15  250.8088  +31.9311
  151  7C 164116.89+320153.00            6.26e+02  1.3e+02      70.20   72764 0   -0.65    4.21  250.7970  +31.9386
  325  WN B1641.2+3201                   3.93e+02  7.9e+01      12.00   72764 0   -0.62    4.15  250.7972  +31.9396
  365  TXS 1641+320                      4.07e+02  8.1e+01       6.00   72764 0   -0.65    4.21  250.7976  +31.9383
  408  B2.1 1641+32                      3.40e+02  6.8e+01       0.00   72764 0   -0.62    4.16  250.7958  +31.9200
 1400  FIRST J164311.3+315618            1.20e+02  2.4e+01       5.00   72764 0   -0.57    3.94  250.7973  +31.9383
 1400  NVSS J164311+315617               1.21e+02  2.4e+01      45.00   72764 0   -0.62    4.15  250.7972  +31.9382
 1400  WB 1641+3201                      1.47e+02  2.9e+01     120.00   72764 0   -0.63    4.16  250.8017  +31.9311
 4850  87GB 164118.4+320129              7.26e+01  1.5e+01     138.00   72764 0   -0.62    4.15  250.8038  +31.9322
 4850  BWE 1641+3201                     7.70e+01  1.5e+01     138.00   72764 0   -0.67    4.29  250.8017  +31.9311
 4850  GB6 B1641+3201                    4.84e+01  9.7e+00     108.00   72764 0   -0.80    4.62  250.8063  +31.9319

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 B1641.3+3159                   3.70e+01  7.4e+00      12.00   -72764  250.8195  +31.8927
   408  B2.1 1641+32                      3.40e+02  6.8e+01       0.00    72764  250.7958  +31.9200
  1400  FIRST J164316.6+315334            1.08e+01  2.2e+00       5.00   -72764  250.8193  +31.8930
  1400  NVSS J164316+315329               1.90e+01  3.8e+00      45.00   -72764  250.8190  +31.8915

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