Complement to VIII/85A

Source MITG_J180356+0340: 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 J1803.9+0341                 1.23e+03  2.5e+02      79.98   75521 0   -0.54    4.13  270.9850  +03.6880
  365  TXS 1801+036                      7.48e+02  1.5e+02       6.00   75521 0   -0.54    4.13  270.9846  +03.6854
 1400  NVSS J180356+034107               2.73e+02  5.5e+01      45.00   75521 0   -0.54    4.13  270.9843  +03.6853
 4850  87GB 180128.4+034031              2.50e+02  5.0e+01     138.00   75521 0   -0.51    4.05  270.9912  +03.6786
 4850  BWE 1801+0340                     2.50e+02  5.0e+01     138.00   75521 0   -0.51    4.05  270.9921  +03.6775
 4850  GB6 B1801+0340                    2.39e+02  4.8e+01     108.00   75521 0   -0.51    4.05  270.9862  +03.6833
 4850  MITG J180356+0340                 2.00e+02  4.0e+01     258.00   75521 0   -0.51    4.05  270.9871  +03.6808
 8400  CLASS J180356.2815+034107.576     1.04e+02  2.1e+01       0.33   75521 0   -0.54    4.13  270.9845  +03.6854
 8400  JVAS J1803+0341                   1.10e+02  2.2e+01       0.33   75521 0   -0.54    4.13  270.9845  +03.6854

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 J1803.9+0341                 1.23e+03  2.5e+02      79.98    75521  270.9850  +03.6880
   365  TXS 1801+036                      7.48e+02  1.5e+02       6.00    75521  270.9846  +03.6854
  1400  NVSS J180356+034107               2.73e+02  5.5e+01      45.00    75521  270.9843  +03.6853
  4850  87GB 180128.4+034031              2.50e+02  5.0e+01     138.00    75521  270.9912  +03.6786
  4850  BWE 1801+0340                     2.50e+02  5.0e+01     138.00    75521  270.9921  +03.6775
  4850  GB6 B1801+0340                    2.39e+02  4.8e+01     108.00    75521  270.9862  +03.6833
  8400  CLASS J180356.2815+034107.576     1.04e+02  2.1e+01       0.33    75521  270.9845  +03.6854

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