Complement to VIII/85A

Source NVSS_J221413-170425: 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 J2214.4-1701                 1.64e+05  3.3e+04      79.98   96886 0   -1.02    7.15  333.6071  -17.0281
   80  Cula 2211-172                     1.46e+05  2.9e+04     222.00   96886 0   -0.99    7.07  333.6029  -17.0314
  160  Culb 2211-172                     7.92e+04  1.6e+04     111.00   96886 0   -1.01    7.10  333.6029  -17.0314
  325  WISH B2211.7-1716                 3.84e+04  7.7e+03      18.00   96886 0   -1.02    7.15  333.6067  -17.0296
  408  MRC 2211-172                      2.87e+04  5.7e+03     120.00   96886 0   -1.02    7.15  333.6067  -17.0289
 2700  PKS J2214-1701                    4.62e+03  9.2e+02      60.00   96886 0   -1.02    7.15  333.6067  -17.0261

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 J2214.4-1701                 1.64e+05  3.3e+04      79.98    96886  333.6071  -17.0281
   160  Culb 2211-172                     7.92e+04  1.6e+04     111.00    96886  333.6029  -17.0314
   325  WISH B2211.7-1716                 3.84e+04  7.7e+03      18.00    96886  333.6067  -17.0296
   365  TXS 2211-172                      1.90e+04  3.8e+03       6.00   -96886  333.6083  -17.0298
   408  MRC 2211-172                      2.87e+04  5.7e+03     120.00    96886  333.6067  -17.0289
  1400  NVSS J221413-170201               4.12e+01  8.2e+00      45.00   -96886  333.5568  -17.0338
  1400  NVSS J221413-170425               2.40e+00  5.0e-01      45.00   -96886  333.5554  -17.0738
  1400  NVSS J221424-170100               4.23e+03  8.5e+02      45.00   -96886  333.6039  -17.0167
  1400  NVSS J221426-170220               4.68e+03  9.4e+02      45.00   -96886  333.6085  -17.0390
  2700  PKS J2214-1701                    4.62e+03  9.2e+02      60.00    96886  333.6067  -17.0261
  4850  PMN J2214-1701                    2.41e+03  4.8e+02     168.00   -96886  333.6075  -17.0308

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