Complement to VIII/85A

Source RGB2_J1221.5+0821: 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 1218+086                      3.17e+02  6.3e+01       6.00   50563 0   -0.45    3.66  185.3845  +08.3615
 1400  FIRST J122132.0+082144            1.50e+02  3.0e+01       5.00   50563 0   -0.45    3.66  185.3836  +08.3622
 1400  NVSS J122132+082143               1.76e+02  3.5e+01      45.00   50563 0   -0.45    3.66  185.3837  +08.3622
 1400  WB 1218+0838                      2.02e+02  4.0e+01     120.00   50563 0   -0.45    3.66  185.3854  +08.3603
 2700  RGB11 J1221.5+0821                1.19e+02  2.4e+01     258.00   50563 0   -0.45    3.66  185.3866  +08.3594
 4850  87GB 121859.8+083813              1.20e+02  2.4e+01     138.00   50563 0   -0.45    3.66  185.3862  +08.3597
 4850  BWE 1218+0838                     1.16e+02  2.3e+01     138.00   50563 0   -0.45    3.66  185.3854  +08.3603
 4850  GB6 B1218+0838                    9.86e+01  2.0e+01     108.00   50563 0   -0.45    3.66  185.3800  +08.3583
 4850  MITG J122131+0821                 1.11e+02  2.2e+01     258.00   50563 0   -0.45    3.66  185.3817  +08.3628
 5000  RGB6 J1221.5+0821                 9.70e+01  1.9e+01     144.00   50563 0   -0.45    3.66  185.3866  +08.3594
10700  RGB2 J1221.5+0821                 7.20e+01  1.4e+01      72.00   50563 0   -0.45    3.66  185.3866  +08.3594

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  


  1400  FIRST J122132.0+082144            1.50e+02  3.0e+01       5.00    50563  185.3836  +08.3622
  1400  NVSS J122132+082143               1.76e+02  3.5e+01      45.00    50563  185.3837  +08.3622
  4850  GB6 B1218+0838                    9.86e+01  2.0e+01     108.00    50563  185.3800  +08.3583
  4885  RGB 1221+083                      5.80e+01  1.2e+01       4.02   -50563  185.3836  +08.3622
  5000  RGB6 J1221.5+0821                 9.70e+01  1.9e+01     144.00    50563  185.3866  +08.3594

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