Complement to VIII/85A

Source MITG_J163046+3612: 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 J1630.7+3613                 6.76e+03  1.4e+03      79.98   68590 4   -0.92    5.62  247.6925  +36.2194
  151  6C 162858+361937                  4.17e+03  8.3e+02     252.00   68590 4   -0.88    5.53  247.6942  +36.2203
  151  7C 162857.79+361934.00            3.78e+03  7.6e+02      70.20   68590 4   -0.88    5.53  247.6925  +36.2194
  232  MY 162858.2+361304.3              3.74e+03  7.5e+02     150.00   68590 4   -0.88    5.53  247.6946  +36.2179
  325  WN B1628.9+3619                   2.22e+03  4.4e+02      12.00   68590 4   -0.92    5.63  247.6930  +36.2194
  365  TXS 1628+363                      1.97e+03  3.9e+02       6.00   68590 4   -0.92    5.63  247.6929  +36.2192
  408  B2.3 1628+36C                     1.68e+03  3.4e+02       0.00   68590 4   -0.88    5.53  247.6908  +36.2233
 1400  NVSS J163046+361310               5.61e+02  1.1e+02      45.00   68590 4   -0.90    5.58  247.6929  +36.2194
 1400  WB 1628+3619                      5.91e+02  1.2e+02     120.00   68590 4   -0.95    5.71  247.6867  +36.2131
 4850  87GB 162856.4+361908              1.59e+02  3.2e+01     138.00   68590 4   -0.88    5.53  247.6871  +36.2122
 4850  BWE 1628+3619                     1.31e+02  2.6e+01     138.00   68590 4   -0.88    5.53  247.6867  +36.2131
 4850  GB6 B1628+3619                    1.43e+02  2.9e+01     108.00   68590 4   -0.88    5.53  247.6896  +36.2169
 4850  MITG J163046+3612                 1.79e+02  3.6e+01     258.00   68590 4   -0.88    5.53  247.6942  +36.2161

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 J1630.7+3613                 6.76e+03  1.4e+03      79.98    68590  247.6925  +36.2194
   151  6C 162858+361937                  4.17e+03  8.3e+02     252.00    68590  247.6942  +36.2203
   178  4C +36.28                         3.60e+03  1.1e+03     690.00   -68590  247.6971  +36.2217
   232  MY 162858.2+361304.3              3.74e+03  7.5e+02     150.00    68590  247.6946  +36.2179
   325  WN B1628.9+3619                   2.22e+03  4.4e+02      12.00    68590  247.6930  +36.2194
   325  WN B1629.3+3616                   7.60e+01  1.5e+01      12.00   -68590  247.7794  +36.1728
   365  TXS 1628+363                      1.97e+03  3.9e+02       6.00    68590  247.6929  +36.2192
   408  B2.3 1628+36C                     1.68e+03  3.4e+02       0.00    68590  247.6908  +36.2233
  1400  FIRST J163020.2+361313            1.40e+00  3.0e-01       5.00   -68590  247.5843  +36.2205
  1400  FIRST J163045.8+361303            1.84e+02  3.7e+01       5.00   -68590  247.6912  +36.2176
  1400  FIRST J163046.2+361307            1.09e+02  2.2e+01       5.00   -68590  247.6926  +36.2188
  1400  FIRST J163046.7+361314            2.51e+02  5.0e+01       5.00   -68590  247.6947  +36.2207
  1400  FIRST J163054.4+361544            1.60e+00  3.0e-01       5.00   -68590  247.7268  +36.2624
  1400  FIRST J163059.9+360821            1.50e+00  3.0e-01       5.00   -68590  247.7498  +36.1392
  1400  FIRST J163103.2+361316            8.00e-01  2.0e-01       5.00   -68590  247.7637  +36.2213
  1400  FIRST J163105.6+361011            5.20e+00  1.0e+00       5.00   -68590  247.7736  +36.1700
  1400  FIRST J163106.2+361016            1.08e+01  2.2e+00       5.00   -68590  247.7758  +36.1713
  1400  FIRST J163107.3+361036            4.00e+00  8.0e-01       5.00   -68590  247.7806  +36.1769
  1400  NVSS J163054+361547               2.40e+00  5.0e-01      45.00   -68590  247.7253  +36.2633
  1400  NVSS J163106+361021               3.28e+01  6.6e+00      45.00   -68590  247.7769  +36.1725
  1400  NVSS J163110+361112               4.90e+00  1.0e+00      45.00   -68590  247.7936  +36.1868
  1400  WB 1628+3619                      5.91e+02  1.2e+02     120.00    68590  247.6867  +36.2131
  4850  87GB 162856.4+361908              1.60e+02  3.2e+01     138.00    68590  247.6871  +36.2122

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