Complement to VIII/85A

Source WN_B0913.6+3830: 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 J0916.7+3818                 2.16e+03  4.3e+02      79.98   39358 4   -0.74    4.78  139.1983  +38.3028
  151  6C 091338+383040                  1.51e+03  3.0e+02     252.00   39358 4   -0.69    4.68  139.1975  +38.3017
  151  7C 091339.20+383042.00            1.47e+03  2.9e+02      70.20   39358 4   -0.74    4.78  139.1992  +38.3022
  232  MY 091339.7+381745.4              8.80e+02  1.8e+02     150.00   39358 4   -0.74    4.78  139.2012  +38.2959
  325  WN B0913.6+3830                   9.24e+02  1.8e+02      12.00   39358 4   -0.74    4.78  139.1997  +38.3014
  325  WN B0913.6+3830A                  8.93e+02  1.8e+02      12.00   39358 4   -0.74    4.78  139.1992  +38.3021
  365  TXS 0913+385                      6.88e+02  1.4e+02       6.00   39358 4   -0.74    4.78  139.1987  +38.3018
  408  B2.3 0913+38                      8.21e+02  1.6e+02       0.00   39358 4   -0.71    4.67  139.2071  +38.2867
  408  B3 0913+385                       7.00e+02  1.4e+02      84.00   39358 4   -0.74    4.78  139.1996  +38.3008
 1400  NVSS J091647+381807               3.34e+02  6.7e+01      45.00   39358 4   -0.74    4.78  139.1992  +38.3021
 1400  WB 0913+3830                      3.36e+02  6.7e+01     120.00   39358 4   -0.72    4.74  139.2004  +38.3019
 4730  B3a 0913+385                      1.41e+02  2.8e+01     168.00   39358 4   -0.68    4.65  139.1995  +38.3010
 4850  87GB 091339.3+383040              1.23e+02  2.5e+01     138.00   39358 4   -0.69    4.68  139.1996  +38.3017
 4850  BWE 0913+3830                     1.19e+02  2.4e+01     138.00   39358 4   -0.74    4.78  139.2004  +38.3019
 4850  GB6 B0913+3830                    1.08e+02  2.2e+01     108.00   39358 4   -0.69    4.68  139.1987  +38.3000
 4850  MITG J091650+3817                 9.40e+01  1.9e+01     258.00   39358 4   -0.75    4.81  139.2104  +38.2867
10600  B3VLA 490                         6.27e+01  1.3e+01      69.00   39358 4   -0.74    4.78  139.1996  +38.3019

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 J0916.7+3818                 2.16e+03  4.3e+02      79.98    39358  139.1983  +38.3028
   151  6C 091338+383040                  1.51e+03  3.0e+02     252.00    39358  139.1975  +38.3017
   232  MY 091339.7+381745.4              8.80e+02  1.8e+02     150.00    39358  139.2012  +38.2959
   325  WN B0913.6+3830A                  8.93e+02  1.8e+02      12.00    39358  139.1992  +38.3021
   325  WN B0913.6+3830B                  2.90e+01  5.8e+00      12.00   -39358  139.2254  +38.2620
   365  TXS 0913+385                      6.88e+02  1.4e+02       6.00    39358  139.1987  +38.3018
   408  B2.3 0913+38                      8.21e+02  1.6e+02       0.00    39358  139.2071  +38.2867
   408  B3 0913+385                       7.00e+02  1.4e+02      84.00    39358  139.1996  +38.3008
  1400  FIRST J091646.8+381806            9.56e+01  1.9e+01       5.00   -39358  139.1951  +38.3019
  1400  FIRST J091647.5+381805            1.04e+02  2.1e+01       5.00   -39358  139.1981  +38.3015
  1400  FIRST J091649.0+381811            9.09e+01  1.8e+01       5.00   -39358  139.2045  +38.3033
  1400  FIRST J091654.2+381556            5.70e+00  1.1e+00       5.00   -39358  139.2261  +38.2658
  1400  FIRST J091654.9+381554            2.80e+00  6.0e-01       5.00   -39358  139.2290  +38.2652
  1400  NVSS J091654+381557               8.80e+00  1.8e+00      45.00   -39358  139.2286  +38.2660
  4730  B3a 0913+385                      1.41e+02  2.8e+01     168.00    39358  139.1995  +38.3010
  4850  GB6 B0913+3830                    1.08e+02  2.2e+01     108.00    39358  139.1987  +38.3000
  4850  MITG J091650+3817                 9.40e+01  1.9e+01     258.00    39358  139.2104  +38.2867
 10600  B3VLA 490                         6.27e+01  1.2e+01      69.00    39358  139.1996  +38.3019

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