Complement to VIII/85A

Source BWE_0325+2911: 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 J0328.6+2921                 4.01e+03  8.0e+02      79.98   10455 5   -0.93    5.51  052.1508  +29.3644
  178  4C +29.10                         3.10e+03  9.3e+02     690.00   10455 5   -0.79    5.14  052.1613  +29.3983
  325  WN B0325.5+2911                   1.49e+03  3.0e+02      12.00   10455 5   -0.83    5.23  052.1499  +29.3663
  365  TXS 0325+291                      1.27e+03  2.5e+02       6.00   10455 5   -0.83    5.23  052.1503  +29.3655
  408  B2.2 0325+29B                     1.04e+03  2.1e+02       0.00   10455 5   -0.79    5.14  052.1496  +29.3633
 1400  NVSS J032836+292157               4.36e+02  8.7e+01      45.00   10455 5   -0.83    5.23  052.1504  +29.3658
 1400  WB 0325+2911                      5.00e+02  1.0e+02     120.00   10455 5   -0.93    5.51  052.1521  +29.3647
 4850  87GB 032533.2+291133              1.49e+02  3.0e+01     138.00   10455 5   -0.79    5.14  052.1517  +29.3647
 4850  BWE 0325+2911                     1.21e+02  2.4e+01     138.00   10455 5   -0.83    5.23  052.1521  +29.3647
 4850  GB6 B0325+2911                    1.43e+02  2.9e+01     108.00   10455 5   -0.79    5.14  052.1504  +29.3658
 4850  MITG J032833+2922                 1.10e+02  2.2e+01     258.00   10455 5   -0.92    5.41  052.1404  +29.3678

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  


   178  4C +29.10                         3.10e+03  9.3e+02     690.00    10455  052.1613  +29.3983
   408  B2.2 0325+29B                     1.04e+03  2.1e+02       0.00    10455  052.1496  +29.3633
  1400  NVSS J032836+292107               7.80e+00  1.6e+00      45.00   -10455  052.1513  +29.3520
  4850  87GB 032533.2+291133              1.49e+02  3.0e+01     138.00    10455  052.1517  +29.3647
  4850  MITG J032833+2922                 1.10e+02  2.2e+01     258.00    10455  052.1404  +29.3678

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