Complement to VIII/85A

Source FIRST_J110854.4+263653: 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 J1108.8+2636                 8.40e+02  1.7e+02      79.98   51644 4   -0.75    4.32  167.2246  +26.6131
  365  TXS 1106+268                      3.61e+02  7.2e+01       6.00   51644 4   -0.70    4.23  167.2224  +26.6140
 1400  NVSS J110853+263649               9.38e+01  1.9e+01      45.00   51644 4   -0.70    4.23  167.2249  +26.6137
 4850  87GB 110612.3+265256              6.23e+01  1.2e+01     138.00   51644 4   -0.70    4.23  167.2237  +26.6111
 4850  BWE 1106+2652                     6.50e+01  1.3e+01     138.00   51644 4   -0.70    4.23  167.2271  +26.6103

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 J1108.8+2636                 8.40e+02  1.7e+02      79.98    51644  167.2246  +26.6131
   365  TXS 1106+268                      3.61e+02  7.2e+01       6.00    51644  167.2224  +26.6140
  1400  FIRST J110846.7+263823            2.70e+00  5.0e-01       5.00   -51644  167.1949  +26.6398
  1400  FIRST J110853.0+263644            3.38e+01  6.8e+00       5.00   -51644  167.2211  +26.6125
  1400  FIRST J110853.7+263636            2.10e+00  4.0e-01       5.00   -51644  167.2240  +26.6101
  1400  FIRST J110854.4+263653            4.26e+01  8.5e+00       5.00   -51644  167.2267  +26.6149
  1400  FIRST J110857.1+263544            1.80e+00  4.0e-01       5.00   -51644  167.2382  +26.5957
  1400  NVSS J110846+263826               3.70e+00  7.0e-01      45.00   -51644  167.1941  +26.6406
  1400  NVSS J110853+263649               9.38e+01  1.9e+01      45.00    51644  167.2249  +26.6137
  4850  87GB 110612.3+265256              6.23e+01  1.2e+01     138.00    51644  167.2237  +26.6111
  4850  BWE 1106+2652                     6.50e+01  1.3e+01     138.00    51644  167.2271  +26.6103
  4850  GB6 B1106+2653                    4.55e+01  9.1e+00     108.00   -51644  167.2254  +26.6150

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