Complement to VIII/85A

Source CLASS_J164029.6332+394646.031A: 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  


  151  6C 163852+395305                  9.90e+02  2.0e+02     252.00   72670 4    0.16    2.52  250.1413  +39.7892
  151  7C 163848.10+395228.00            7.54e+02  1.5e+02      70.20   72670 4    0.16    2.52  250.1229  +39.7789
  365  TXS 1638+398                      8.54e+02  1.7e+02       6.00   72670 4    0.16    2.54  250.1232  +39.7793
  408  B3 1638+398                       7.50e+02  1.5e+02      84.00   72670 4    0.16    2.54  250.1258  +39.7814
 1400  FIRST J164029.6+394645            1.11e+03  2.2e+02       5.00   72670 4    0.16    2.54  250.1235  +39.7794
 1400  NVSS J164029+394646               9.76e+02  2.0e+02      45.00   72670 4    0.14    2.57  250.1236  +39.7795
 1400  WB 1638+3952                      6.57e+02  1.3e+02     120.00   72670 4    0.30    1.93  250.1225  +39.7847
 4730  B3a 1638+398                      1.29e+03  2.6e+02     168.00   72670 4    0.16    2.54  250.1259  +39.7816
 4850  87GB 163848.0+395248              1.28e+03  2.6e+02     138.00   72670 4    0.16    2.54  250.1229  +39.7844
 4850  BWE 1638+3952                     1.27e+03  2.5e+02     138.00   72670 4    0.16    2.54  250.1225  +39.7847
 4850  GB6 B1638+3952                    1.12e+03  2.2e+02     108.00   72670 4    0.10    2.67  250.1229  +39.7844
 4850  MITG J164027+3946                 1.21e+03  2.4e+02     258.00   72670 4    0.16    2.54  250.1154  +39.7806
 8400  CLASS J164029.6332+394646.031A    1.76e+03  3.5e+02       0.33   72670 4    0.16    2.54  250.1235  +39.7795
 8400  CLASS J164029.6332+394646.031B    1.75e+03  3.5e+02       0.33   72670 4    0.16    2.54  250.1235  +39.7795
 8400  CLASS J164029.6332+394646.031C    1.44e+03  2.9e+02       0.33   72670 4    0.16    2.52  250.1235  +39.7795
 8400  CLASS J164029.6332+394646.031D    1.66e+03  3.3e+02       0.33   72670 4    0.16    2.54  250.1235  +39.7795
 8400  JVAS J1640+397                    1.77e+03  3.5e+02       0.33   72670 4    0.16    2.54  250.1235  +39.7795

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 J1640.4+3946                 1.02e+03  2.0e+02      79.98   -72670  250.1242  +39.7819
   151  6C 163852+395305                  9.90e+02  2.0e+02     252.00    72670  250.1413  +39.7892
   151  7C 163848.10+395228.00            7.54e+02  1.5e+02      70.20    72670  250.1229  +39.7789
   232  MY 163851.6+394708.0              4.30e+02  8.6e+01     150.00   -72670  250.1375  +39.7856
   325  WN B1638.8+3952                   6.37e+02  1.3e+02      12.00   -72670  250.1236  +39.7796
   325  WN B1639.0+3954                   4.80e+01  9.6e+00      12.00   -72670  250.1756  +39.8074
   365  TXS 1638+398                      8.54e+02  1.7e+02       6.00    72670  250.1232  +39.7793
   408  B3 1638+398                       7.50e+02  1.5e+02      84.00    72670  250.1258  +39.7814
  1400  FIRST J164029.6+394645            1.11e+03  2.2e+02       5.00    72670  250.1235  +39.7794
  1400  FIRST J164042.0+394825            1.72e+01  3.4e+00       5.00   -72670  250.1753  +39.8071
  1400  NVSS J164029+394646               9.76e+02  2.0e+02      45.00    72670  250.1236  +39.7795
  1400  NVSS J164041+394827               1.06e+01  2.1e+00      45.00   -72670  250.1730  +39.8077
  1400  WB 1638+3952                      6.57e+02  1.3e+02     120.00    72670  250.1225  +39.7847
  1465  [P82] 1638+398                    4.20e+02  8.4e+01      25.80   -72670  250.1232  +39.7794
  4730  B3a 1638+398                      1.29e+03  2.6e+02     168.00    72670  250.1259  +39.7816
  4850  MITG J164027+3946                 1.21e+03  2.4e+02     258.00    72670  250.1154  +39.7806
  4885  [P82a] 1638+398                   8.20e+02  1.6e+02       6.00   -72670  250.1232  +39.7794
  8400  CLASS J164029.6332+394646.031D    1.66e+03  3.3e+02       0.33    72670  250.1235  +39.7795

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