Complement to VIII/85A

Source WN_B0745.6+5209: 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 J0749.4+5202                 2.60e+03  5.2e+02      79.98   31924 5   -0.67    4.75  117.3617  +52.0367
  151  6C 074536+520957                  2.11e+03  4.2e+02     252.00   31924 5   -0.67    4.75  117.3621  +52.0400
  151  7C 074538.20+520953.00            1.98e+03  4.0e+02      70.20   31924 5   -0.43    4.15  117.3688  +52.0389
  232  MY 074536.0+520216.1              1.17e+03  2.3e+02     150.00   31924 5   -0.43    4.15  117.3596  +52.0378
  325  WN B0745.6+5209                   1.31e+03  2.6e+02      12.00   31924 5   -0.67    4.75  117.3638  +52.0378
 1400  ACO 595                           5.20e+02  1.0e+02      15.00   31924 5   -0.67    4.75  117.3654  +52.0414
 1400  ACOa 595                          5.20e+02  1.0e+02     600.00   31924 5   -0.67    4.75  117.3462  +52.0386
 1400  NVSS J074923+520219               2.67e+02  5.3e+01      45.00   31924 5   -0.70    4.72  117.3480  +52.0388
 1400  WB 0745+5210                      5.32e+02  1.1e+02     120.00   31924 5   -0.65    4.72  117.3650  +52.0456
 4850  87GB 074537.1+521017              2.09e+02  4.2e+01     138.00   31924 5   -0.70    4.91  117.3642  +52.0456
 4850  BWE 0745+5210                     2.05e+02  4.1e+01     138.00   31924 5   -0.67    4.75  117.3650  +52.0456
 4850  GB6 B0745+5210                    1.97e+02  3.9e+01     108.00   31924 5   -0.43    4.15  117.3650  +52.0439

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 J0749.4+5202                 2.60e+03  5.2e+02      79.98    31924  117.3617  +52.0367
   151  7C 074538.20+520953.00            1.98e+03  4.0e+02      70.20    31924  117.3688  +52.0389
   232  MY 074536.0+520216.1              1.17e+03  2.3e+02     150.00    31924  117.3596  +52.0378
   325  WN B0745.4+5212                   2.70e+01  5.4e+00      12.00   -31924  117.3309  +52.0761
   325  WN B0745.6+5209                   1.31e+03  2.6e+02      12.00    31924  117.3638  +52.0378
   325  WN B0745.6+5209A                  6.89e+02  1.4e+02      12.00   -31924  117.3493  +52.0383
   325  WN B0745.6+5209B                  6.19e+02  1.2e+02      12.00   -31924  117.3800  +52.0372
   365  TXS 0745+521                      5.81e+02  1.2e+02       6.00   -31924  117.3417  +52.0393
  1400  ACOa 595                          5.20e+02  1.0e+02     600.00    31924  117.3462  +52.0386
  1400  FIRST J074922.0+520216            4.35e+01  8.7e+00       5.00   -31924  117.3419  +52.0379
  1400  FIRST J074922.3+520227            5.90e+01  1.2e+01       5.00   -31924  117.3432  +52.0410
  1400  FIRST J074923.9+520212            6.37e+01  1.3e+01       5.00   -31924  117.3498  +52.0367
  1400  FIRST J074924.6+520141            8.20e+00  1.6e+00       5.00   -31924  117.3526  +52.0281
  1400  FIRST J074926.1+520230            4.47e+01  8.9e+00       5.00   -31924  117.3589  +52.0419
  1400  FIRST J074930.4+520209            4.35e+01  8.7e+00       5.00   -31924  117.3770  +52.0358
  1400  FIRST J074931.4+520222            5.70e+01  1.1e+01       5.00   -31924  117.3812  +52.0395
  1400  FIRST J074932.2+520223            4.23e+01  8.5e+00       5.00   -31924  117.3845  +52.0399
  1400  FIRST J074932.8+520219            5.81e+01  1.2e+01       5.00   -31924  117.3869  +52.0386
  1400  FIRST J074932.8+520232            8.10e+00  1.6e+00       5.00   -31924  117.3869  +52.0424
  1400  NVSS J074918+520431               7.50e+00  1.5e+00      45.00   -31924  117.3278  +52.0754
  1400  NVSS J074923+520219               2.67e+02  5.3e+01      45.00    31924  117.3480  +52.0388
  1400  NVSS J074927+520131               1.19e+01  2.4e+00      45.00   -31924  117.3638  +52.0255
  4850  GB6 B0745+5210                    1.97e+02  3.9e+01     108.00    31924  117.3650  +52.0439
  8400  CLASS J074927.2442+520232.518     8.70e+00  1.7e+00       0.33   -31924  117.3635  +52.0424

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