Complement to VIII/85A

Source WN_B0721.5+3927: 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 J0724.9+3921                 8.30e+02  1.7e+02      79.98   31059 1   -0.74    4.27  111.2475  +39.3575
  151  7C 072134.50+392718.00            4.98e+02  1.0e+02      70.20   31059 1   -0.74    4.27  111.2479  +39.3561
  232  MY 072131.4+392158.3              4.10e+02  1.1e+02     150.00   31059 1   -0.77    4.38  111.2354  +39.3662
  232  MY 072136.3+392054.6              3.10e+02  6.2e+01     150.00   31059 1   -0.76    4.35  111.2554  +39.3485
  325  WN B0721.5+3927                   2.86e+02  5.7e+01      12.00   31059 1   -0.74    4.27  111.2474  +39.3561
  408  B3 0721+394                       2.00e+02  4.0e+01      84.00   31059 1   -0.74    4.27  111.2529  +39.3544
 1400  FIRST J072459.3+392123            8.65e+01  1.7e+01       5.00   31059 1   -0.74    4.27  111.2472  +39.3564
 1400  NVSS J072459+392123               8.48e+01  1.7e+01      45.00   31059 1   -0.74    4.27  111.2466  +39.3566
 4850  87GB 072134.3+392730              3.40e+01  6.8e+00     138.00   31059 1   -0.74    4.27  111.2471  +39.3594
 4850  BWE 0721+3927                     3.60e+01  7.2e+00     138.00   31059 1   -0.74    4.27  111.2500  +39.3639
 4850  GB6 B0721+3927                    3.20e+01  6.4e+00     108.00   31059 1   -0.78    4.37  111.2471  +39.3597
10600  B3VLA 309                         1.88e+01  3.8e+00      69.00   31059 1   -0.74    4.27  111.2471  +39.3561

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  


   232  MY 072136.3+392054.6              3.10e+02  6.2e+01     150.00    31059  111.2554  +39.3485
  1400  FIRST J072506.8+392114            2.30e+00  5.0e-01       5.00   -31059  111.2784  +39.3541
  1400  NVSS J072506+392126               3.10e+00  6.0e-01      45.00   -31059  111.2770  +39.3574
  4850  87GB 072134.3+392730              3.40e+01  6.8e+00     138.00    31059  111.2471  +39.3594

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