Complement to VIII/85A

Source B3_1030+415: 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 J1033.0+4116                 1.14e+03  2.3e+02      79.98   41912 0   -0.23    3.50  158.2663  +41.2672
  151  7C 103008.00+413135.00            1.29e+03  2.6e+02      70.20   41912 0   -0.23    3.50  158.2662  +41.2683
  232  MY 103009.0+411601.5              8.90e+02  1.8e+02     150.00   41912 0   -0.23    3.50  158.2704  +41.2671
  325  WN B1030.1+4131                   7.74e+02  1.5e+02      12.00   41912 0   -0.23    3.50  158.2657  +41.2683
  365  TXS 1030+415                      8.54e+02  1.7e+02       6.00   41912 0   -0.23    3.50  158.2659  +41.2683
  408  B3 1030+415                       1.02e+03  2.0e+02      84.00   41912 0   -0.23    3.50  158.2667  +41.2683
 1400  FIRST J103303.7+411606            4.33e+02  8.7e+01       5.00   41912 0   -0.16    3.24  158.2655  +41.2684
 1400  NVSS J103303+411606               4.73e+02  9.5e+01      45.00   41912 0   -0.16    3.24  158.2655  +41.2685
 1400  WB 1030+4131                      7.73e+02  1.5e+02     120.00   41912 0   -0.20    3.45  158.2692  +41.2664
 1465  [P82] 1030+415                    6.30e+02  1.3e+02      25.80   41912 0   -0.23    3.50  158.2653  +41.2683
 4730  B3a 1030+415                      5.93e+02  1.2e+02     168.00   41912 0   -0.26    3.59  158.2665  +41.2683
 4850  87GB 103008.2+413131              5.48e+02  1.1e+02     138.00   41912 0   -0.23    3.50  158.2671  +41.2675
 4850  BWE 1030+4131                     5.08e+02  1.0e+02     138.00   41912 0   -0.23    3.50  158.2692  +41.2664
 4850  GB6 B1030+4131                    4.39e+02  8.8e+01     108.00   41912 0   -0.26    3.59  158.2663  +41.2664
 4885  [P82a] 1030+415                   5.80e+02  1.2e+02       6.00   41912 0   -0.26    3.59  158.2653  +41.2683
 8400  CLASS J103303.7086+411606.233A    3.87e+02  7.7e+01       0.33   41912 0   -0.23    3.50  158.2654  +41.2684
 8400  CLASS J103303.7086+411606.233B    3.81e+02  7.6e+01       0.33   41912 0   -0.23    3.50  158.2654  +41.2684
 8400  JVAS J1033+412                    3.78e+02  7.6e+01       0.33   41912 0   -0.23    3.50  158.2655  +41.2684

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 J1033.0+4116                 1.14e+03  2.3e+02      79.98    41912  158.2663  +41.2672
   151  6C 103007+413130                  2.01e+03  4.0e+02     252.00   -41912  158.2658  +41.2672
   151  7C 103008.00+413135.00            1.29e+03  2.6e+02      70.20    41912  158.2662  +41.2683
   232  MY 103009.0+411601.5              8.90e+02  1.8e+02     150.00    41912  158.2704  +41.2671
   325  WN B1030.1+4131                   7.74e+02  1.5e+02      12.00    41912  158.2657  +41.2683
   365  TXS 1030+415                      8.54e+02  1.7e+02       6.00    41912  158.2659  +41.2683
   408  B3 1030+415                       1.02e+03  2.0e+02      84.00    41912  158.2667  +41.2683
  1400  FIRST J103302.1+411643            1.40e+00  3.0e-01       5.00   -41912  158.2591  +41.2789
  1400  FIRST J103303.4+411555            1.90e+00  4.0e-01       5.00   -41912  158.2643  +41.2655
  1400  FIRST J103303.7+411606            4.33e+02  8.6e+01       5.00    41912  158.2655  +41.2684
  1400  NVSS J103303+411606               4.73e+02  9.5e+01      45.00    41912  158.2655  +41.2685
  1400  WB 1030+4131                      7.73e+02  1.5e+02     120.00    41912  158.2692  +41.2664
  4730  B3a 1030+415                      5.93e+02  1.2e+02     168.00    41912  158.2665  +41.2683
  4850  GB6 B1030+4131                    4.39e+02  8.8e+01     108.00    41912  158.2663  +41.2664
  4885  [P82a] 1030+415                   5.80e+02  1.2e+02       6.00    41912  158.2653  +41.2683
  8400  CLASS J103303.7086+411606.233B    3.81e+02  7.6e+01       0.33    41912  158.2654  +41.2684
 10600  B3VLA 588                         2.30e+02  4.6e+01      69.00   -41912  158.2654  +41.2681

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