Complement to VIII/85A

Source WB_2258+1924: 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 J2301.2+1940                 1.02e+04  2.0e+03      79.98   93641 0   -0.85    5.60  345.3233  +19.6730
   80  Cula 2258+193                     1.10e+04  2.2e+03     222.00   93641 0   -0.86    5.62  345.3208  +19.6578
  160  Culb 2258+193                     5.40e+03  1.1e+03     111.00   93641 0   -0.86    5.62  345.3208  +19.6578
  178  4C +19.75                         4.80e+03  1.4e+03     690.00   93641 0   -0.86    5.62  345.3221  +19.6600
  365  TXS 2258+194                      3.35e+03  6.7e+02       6.00   93641 0   -0.85    5.60  345.3225  +19.6719
 1400  WB 2258+1924                      8.77e+02  1.8e+02     120.00   93641 0   -0.85    5.60  345.3242  +19.6744
 2700  PKS J2301+1940                    4.00e+02  8.0e+01      60.00   93641 0   -0.86    5.62  345.3225  +19.6714
 4850  87GB 225850.1+192419              2.77e+02  5.5e+01     138.00   93641 0   -0.87    5.65  345.3238  +19.6742
 4850  BWE 2258+1924                     2.73e+02  5.5e+01     138.00   93641 0   -0.87    5.63  345.3242  +19.6744
 4850  GB6 B2258+1924                    2.94e+02  5.9e+01     108.00   93641 0   -0.85    5.61  345.3221  +19.6733
 4850  MITG J230118+1939                 2.91e+02  5.8e+01     258.00   93641 0   -0.86    5.62  345.3275  +19.6569
 4850  MITG J230119+1939                 3.00e+02  6.0e+01     258.00   93641 0   -0.85    5.60  345.3300  +19.6614

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 J2301.2+1940                 1.02e+04  2.0e+03      79.98    93641  345.3233  +19.6730
   178  4C +19.75                         4.80e+03  1.4e+03     690.00    93641  345.3221  +19.6600
  1400  NVSS J230119+194036               4.54e+02  9.1e+01      45.00   -93641  345.3292  +19.6767
  4850  MITG J230118+1939                 2.91e+02  5.8e+01     258.00    93641  345.3275  +19.6569

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