Complement to VIII/85A

Source MITG_J210808+2139: 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 J2108.1+2140                 9.30e+03  1.9e+03      79.98   87337 5   -0.99    5.83  317.0321  +21.6730
   80  Cula 2105+214                     7.00e+03  1.4e+03     222.00   87337 5   -0.95    5.74  317.0304  +21.6661
  160  Culb 2105+214                     4.40e+03  8.8e+02     111.00   87337 5   -0.99    5.83  317.0304  +21.6661
  178  4C +21.58                         4.30e+03  1.3e+03     690.00   87337 5   -0.95    5.75  317.0362  +21.6767
  365  TXS 2105+214                      2.40e+03  4.8e+02       6.00   87337 5   -0.95    5.75  317.0317  +21.6731
 1400  NVSS J210807+214025               5.80e+02  1.2e+02      45.00   87337 5   -0.99    5.83  317.0303  +21.6736
 1400  WB 2105+2128                      5.12e+02  1.0e+02     120.00   87337 5   -0.95    5.75  317.0350  +21.6731
 2700  PKS J2108+2140                    3.00e+02  6.0e+01      60.00   87337 5   -0.95    5.75  317.0342  +21.6700
 4850  87GB 210552.5+212813              1.53e+02  3.1e+01     138.00   87337 5   -0.95    5.75  317.0342  +21.6731
 4850  BWE 2105+2128                     1.31e+02  2.6e+01     138.00   87337 5   -0.95    5.75  317.0350  +21.6731
 4850  GB6 B2105+2128                    1.40e+02  2.8e+01     108.00   87337 5   -0.95    5.75  317.0333  +21.6742
 4850  MITG J210808+2139                 1.38e+02  2.8e+01     258.00   87337 5   -0.95    5.75  317.0371  +21.6636

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  


   160  Culb 2105+214                     4.40e+03  8.8e+02     111.00    87337  317.0304  +21.6661
   178  4C +21.58                         4.30e+03  1.3e+03     690.00    87337  317.0362  +21.6767
  1400  NVSS J210810+213956               4.34e+01  8.7e+00      45.00   -87337  317.0452  +21.6657
  4850  MITG J210808+2139                 1.38e+02  2.8e+01     258.00    87337  317.0371  +21.6636

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