Complement to VIII/85A

Source WB_0833+5835A: 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 083326+583448                  7.60e+02  1.5e+02     252.00   33656 0   -0.05    2.99  129.3525  +58.4053
  151  7C 083324.39+583523.00            7.66e+02  1.5e+02      70.20   33656 0    0.11    2.45  129.3462  +58.4150
  365  TXS 0833+585                      8.16e+02  1.6e+02       6.00   33656 0    0.08    2.52  129.3442  +58.4169
 1400  FIRST J083722.4+582501            6.88e+02  1.4e+02       5.00   33656 0    0.03    2.73  129.3434  +58.4172
 1400  NVSS J083722+582501               6.90e+02  1.4e+02      45.00   33656 0    0.24    2.08  129.3435  +58.4170
 1400  WB 0833+5835A                     5.97e+02  1.2e+02     120.00   33656 0    0.24    2.08  129.3338  +58.4208
 1465  [P82] 0833+585                    5.70e+02  1.1e+02      25.80   33656 0    0.11    2.45  129.3434  +58.4171
 2700  RGB11 J0837.4+5825                6.67e+02  1.3e+02     258.00   33656 0   -0.05    2.99  129.3371  +58.4211
 4850  87GB 083322.1+583544              7.56e+02  1.5e+02     138.00   33656 0   -0.05    2.99  129.3367  +58.4211
 4850  BWE 0833+5835A                    6.61e+02  1.3e+02     138.00   33656 0   -0.05    2.99  129.3338  +58.4208
 4850  GB6 B0833+5835                    7.17e+02  1.4e+02     108.00   33656 0   -0.05    2.99  129.3363  +58.4206
 4885  [P82a] 0833+585                   1.23e+03  2.5e+02       6.00   33656 0    0.24    2.08  129.3434  +58.4171
 4885  RGB 0837+584                      7.17e+02  1.4e+02       4.02   33656 0   -0.05    2.99  129.3433  +58.4172
 5000  RGB6 J0837.4+5825                 5.57e+02  1.1e+02     144.00   33656 0   -0.05    2.98  129.3371  +58.4211
 8400  CLASS J083722.4090+582501.844     5.10e+02  1.0e+02       0.33   33656 0   -0.05    2.99  129.3433  +58.4172
 8400  CLASS J083722.4126+582501.830     4.98e+02  1.0e+02       0.33   33656 0   -0.05    2.99  129.3434  +58.4172
 8400  JVAS J0837+584                    4.97e+02  9.9e+01       0.33   33656 0   -0.05    2.99  129.3434  +58.4172
10700  RGB2 J0837.4+5825                 7.80e+02  1.6e+02      72.00   33656 0    0.11    2.45  129.3371  +58.4211

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  


   151  6C 083326+583448                  7.60e+02  1.5e+02     252.00    33656  129.3525  +58.4053
   151  7C 083324.39+583523.00            7.66e+02  1.5e+02      70.20    33656  129.3462  +58.4150
   232  MY 083321.0+582514.3              2.80e+02  6.8e+01     150.00   -33656  129.3321  +58.4206
   232  MY 083326.8+582355.8              3.90e+02  1.1e+02     150.00   -33656  129.3558  +58.3988
   325  WN B0833.3+5835                   5.31e+02  1.1e+02      12.00   -33656  129.3438  +58.4167
   365  TXS 0833+585                      8.16e+02  1.6e+02       6.00    33656  129.3442  +58.4169
  1400  FIRST J083715.7+582450            1.00e+00  2.0e-01       5.00   -33656  129.3156  +58.4140
  1400  FIRST J083724.2+582543            1.10e+00  2.0e-01       5.00   -33656  129.3512  +58.4288
  1400  FIRST J083728.2+582505            2.10e+00  4.0e-01       5.00   -33656  129.3678  +58.4181
  1400  NVSS J083722+582501               6.90e+02  1.4e+02      45.00    33656  129.3435  +58.4170
  1400  WB 0833+5835A                     5.97e+02  1.2e+02     120.00    33656  129.3338  +58.4208
  4850  87GB 083322.1+583544              7.56e+02  1.5e+02     138.00    33656  129.3367  +58.4211
  4850  GB6 B0833+5835                    7.17e+02  1.4e+02     108.00    33656  129.3363  +58.4206
  4885  [P82a] 0833+585                   1.23e+03  2.5e+02       6.00    33656  129.3434  +58.4171
  4885  RGB 0837+584                      7.17e+02  1.4e+02       4.02    33656  129.3433  +58.4172
  5000  RGB6 J0837.4+5825                 5.57e+02  1.1e+02     144.00    33656  129.3371  +58.4211
  8400  CLASS J083722.4090+582501.844     5.10e+02  1.0e+02       0.33    33656  129.3433  +58.4172

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