Complement to VIII/85A

Source VLSS_J1210.1+3821: 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 J1210.1+3821                 3.05e+03  6.1e+02      79.98   50193 0   -0.84    5.14  182.5392  +38.3547
  151  6C 120737+383757                  2.15e+03  4.3e+02     252.00   50193 0   -0.83    5.15  182.5379  +38.3544
  151  7C 120737.60+383757.00            2.06e+03  4.1e+02      70.20   50193 0   -0.84    5.16  182.5387  +38.3542
  325  WN B1207.6+3837                   1.23e+03  2.5e+02      12.00   50193 0   -0.84    5.14  182.5383  +38.3540
  325  WN B1207.6+3837B                  1.21e+03  2.4e+02      12.00   50193 0   -0.88    5.22  182.5387  +38.3541
  365  TXS 1207+386                      1.15e+03  2.3e+02       6.00   50193 0   -0.85    5.19  182.5388  +38.3539
  408  B2.3 1207+38                      1.06e+03  2.1e+02       0.00   50193 0   -0.83    5.15  182.5392  +38.3350
  408  B3 1207+386                       9.40e+02  1.9e+02      84.00   50193 0   -0.84    5.14  182.5396  +38.3561
 1400  NVSS J121009+382114               3.46e+02  6.9e+01      45.00   50193 0   -0.85    5.19  182.5390  +38.3539
 1400  WB 1207+3837                      3.35e+02  6.7e+01     120.00   50193 0   -0.81    5.07  182.5450  +38.3536
 4730  B3a 1207+386                      1.14e+02  2.3e+01     168.00   50193 0   -0.89    5.32  182.5393  +38.3561
 4850  87GB 120739.0+383754              1.43e+02  2.9e+01     138.00   50193 0   -0.74    4.87  182.5446  +38.3536
 4850  BWE 1207+3837                     1.25e+02  2.5e+01     138.00   50193 0   -0.82    5.12  182.5450  +38.3536
 4850  GB6 B1207+3837                    9.90e+01  2.0e+01     108.00   50193 0   -0.89    5.32  182.5417  +38.3533
10600  B3VLA 726                         3.84e+01  7.7e+00      69.00   50193 0   -0.84    5.14  182.5387  +38.3536

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 J1210.1+3821                 3.05e+03  6.1e+02      79.98    50193  182.5392  +38.3547
   151  6C 120737+383757                  2.15e+03  4.3e+02     252.00    50193  182.5379  +38.3544
   232  MY 120736.9+382112.1              9.70e+02  1.9e+02     150.00   -50193  182.5358  +38.3534
   325  WN B1207.6+3837                   1.23e+03  2.5e+02      12.00    50193  182.5383  +38.3540
   325  WN B1207.6+3837A                  2.10e+01  4.2e+00      12.00   -50193  182.4987  +38.3442
   365  TXS 1207+386                      1.15e+03  2.3e+02       6.00    50193  182.5388  +38.3539
   408  B2.3 1207+38                      1.06e+03  2.1e+02       0.00    50193  182.5392  +38.3350
   408  B3 1207+386                       9.40e+02  1.9e+02      84.00    50193  182.5396  +38.3561
  1400  FIRST J120957.7+382337            5.40e+00  1.1e+00       5.00   -50193  182.4906  +38.3936
  1400  FIRST J120959.7+382046            7.70e+00  1.5e+00       5.00   -50193  182.4989  +38.3463
  1400  FIRST J121008.3+382113            1.44e+02  2.9e+01       5.00   -50193  182.5346  +38.3537
  1400  FIRST J121010.4+382116            1.45e+02  2.9e+01       5.00   -50193  182.5436  +38.3544
  1400  NVSS J120957+382334               6.20e+00  1.2e+00      45.00   -50193  182.4902  +38.3930
  1400  NVSS J120959+382045               7.50e+00  1.5e+00      45.00   -50193  182.4973  +38.3461
  1400  NVSS J121009+382114               3.46e+02  6.9e+01      45.00    50193  182.5390  +38.3539
  1400  WB 1207+3837                      3.35e+02  6.7e+01     120.00    50193  182.5450  +38.3536
  4730  B3a 1207+386                      1.14e+02  2.3e+01     168.00    50193  182.5393  +38.3561
  4850  87GB 120739.0+383754              1.43e+02  2.9e+01     138.00    50193  182.5446  +38.3536
  4850  GB6 B1207+3837                    9.90e+01  2.0e+01     108.00    50193  182.5417  +38.3533
  4850  MITG J121002+3822                 5.80e+01  1.2e+01     258.00   -50193  182.5117  +38.3694
 10600  B3VLA 726                         3.84e+01  7.7e+00      69.00    50193  182.5387  +38.3536

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