Complement to VIII/85A

Source BWE_2250+0220: 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  


 1400  NVSS J225321+023612               2.93e+02  5.9e+01      45.00   93374 0    0.00    2.45  343.3378  +02.6035
 1400  WB 2250+0220                      2.71e+02  5.4e+01     120.00   93374 0    0.00    2.45  343.3379  +02.6000
 2700  PKS J2253+0236                    3.10e+02  6.2e+01      60.00   93374 0    0.00    2.45  343.3375  +02.6053
 4850  87GB 225048.1+022000              2.94e+02  5.9e+01     138.00   93374 0   -0.24    3.24  343.3375  +02.5994
 4850  BWE 2250+0220                     2.36e+02  4.7e+01     138.00   93374 0   -0.11    2.78  343.3379  +02.6000
 4850  GB6 B2250+0220                    2.94e+02  5.9e+01     108.00   93374 0   -0.24    3.24  343.3375  +02.6042
 4850  MITG J225323+0235                 2.86e+02  5.7e+01     258.00   93374 0    0.04    2.30  343.3462  +02.5956
 4850  PMN J2253+0236                    2.48e+02  5.0e+01     168.00   93374 0    0.00    2.45  343.3413  +02.6022
 8400  CLASS J225321.1002+023613.050     1.86e+02  3.7e+01       0.33   93374 0   -0.24    3.24  343.3379  +02.6036
 8400  JVAS J2253+0236                   1.96e+02  3.9e+01       0.33   93374 0    0.00    2.45  343.3379  +02.6036

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  


  1400  NVSS J225311+024013               3.14e+01  6.3e+00      45.00   -93374  343.2969  +02.6705
  1400  NVSS J225335+023340               5.60e+00  1.1e+00      45.00   -93374  343.3981  +02.5614
  1400  WB 2250+0220                      2.71e+02  5.4e+01     120.00    93374  343.3379  +02.6000
  2700  PKS J2253+0236                    3.10e+02  6.2e+01      60.00    93374  343.3375  +02.6053
  4850  PMN J2253+0236                    2.48e+02  5.0e+01     168.00    93374  343.3413  +02.6022
  8400  JVAS J2253+0236                   1.96e+02  3.9e+01       0.33    93374  343.3379  +02.6036

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