Complement to VIII/85A

Source FIRST_J112835.5+210237: 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  


  365  TXS 1125+213                      4.40e+02  8.8e+01       6.00   48769 0   -0.41    3.95  172.1474  +21.0432
 1400  FIRST J112835.5+210237            2.64e+02  5.3e+01       5.00   48769 0   -0.41    3.95  172.1481  +21.0437
 1400  NVSS J112835+210236               2.92e+02  5.8e+01      45.00   48769 0   -0.41    3.95  172.1482  +21.0436
 4850  87GB 112554.9+211848              2.53e+02  5.1e+01     138.00   48769 0   -0.15    2.95  172.1346  +21.0378
 4850  BWE 1125+2118                     2.47e+02  4.9e+01     138.00   48769 0   -0.41    3.95  172.1354  +21.0372
 4850  GB6 B1125+2119                    2.20e+02  4.4e+01     108.00   48769 0   -0.41    3.95  172.1450  +21.0433
 4850  MITG J112837+2102                 2.39e+02  4.8e+01     258.00   48769 0   -0.41    3.95  172.1567  +21.0386
 8400  CLASS J112835.5459+210237.393     2.22e+02  4.4e+01       0.33   48769 0   -0.41    3.95  172.1481  +21.0437
 8400  JVAS J1128+2102                   2.14e+02  4.3e+01       0.33   48769 0   -0.42    3.96  172.1481  +21.0437

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 J1128.5+2102                 1.53e+03  3.1e+02      79.98   -48769  172.1454  +21.0446
   365  TXS 1125+213                      4.40e+02  8.8e+01       6.00    48769  172.1474  +21.0432
  1400  FIRST J112835.5+210237            2.64e+02  5.3e+01       5.00    48769  172.1481  +21.0437
  1400  FIRST J112836.1+210246            7.90e+00  1.6e+00       5.00   -48769  172.1507  +21.0461
  1400  NVSS J112835+210236               2.92e+02  5.8e+01      45.00    48769  172.1482  +21.0436
  4850  87GB 112554.9+211848              2.53e+02  5.1e+01     138.00    48769  172.1346  +21.0378
  8400  CLASS J112835.5459+210237.393     2.22e+02  4.4e+01       0.33    48769  172.1481  +21.0437

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