Complement to VIII/85A

Source Cula_1232-249: 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 J1235.6-2511                 2.50e+04  5.0e+03      79.98   52544 0   -0.87    6.03  188.9058  -25.2000
   80  Cula 1232-249                     2.60e+04  5.2e+03     222.00   52544 0   -0.83    5.88  188.9058  -25.2011
  160  Culb 1232-249                     1.17e+04  2.3e+03     111.00   52544 0   -0.87    6.03  188.9058  -25.2011
  325  WISH B1232.9-2455                 6.36e+03  1.3e+03      18.00   52544 0   -0.87    6.03  188.9075  -25.2049
  325  WISH B1232.9-2455A                4.91e+03  9.8e+02      18.00   52544 0   -0.87    6.03  188.9061  -25.1974
  365  TXS 1232-249                      6.80e+03  1.4e+03       6.00   52544 0   -0.87    6.03  188.9073  -25.2029
  408  MRC 1232-249                      5.10e+03  1.0e+03     120.00   52544 0   -0.87    6.03  188.9067  -25.2028
 2700  PKS J1235-2512                    1.10e+03  2.2e+02      60.00   52544 0   -0.83    5.88  188.9075  -25.2047
 4850  PMN J1235-2512                    6.52e+02  1.3e+02     168.00   52544 0   -0.89    6.02  188.9117  -25.2069

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 J1235.6-2511                 2.50e+04  5.0e+03      79.98    52544  188.9058  -25.2000
   325  WISH B1232.9-2455A                4.91e+03  9.8e+02      18.00    52544  188.9061  -25.1974
   325  WISH B1232.9-2455B                1.45e+03  2.9e+02      18.00   -52544  188.9123  -25.2307
   408  MRC 1232-249                      5.10e+03  1.0e+03     120.00    52544  188.9067  -25.2028
  1400  NVSS J123536-251126               1.20e+03  2.4e+02      45.00   -52544  188.9033  -25.1906
  1400  NVSS J123538-251302               9.80e+02  2.0e+02      45.00   -52544  188.9116  -25.2174
  4850  PMN J1235-2512                    6.52e+02  1.3e+02     168.00    52544  188.9117  -25.2069

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