Complement to VIII/85A

Source MITG_J214410+1930: 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 J2144.1+1929                 6.96e+03  1.4e+03      79.98   88540 0   -1.06    5.83  326.0308  +19.4869
  178  4C +19.71                         2.50e+03  7.5e+02     690.00   88540 0   -1.06    5.83  326.0317  +19.4817
  365  TXS 2141+192                      1.61e+03  3.2e+02       6.00   88540 0   -1.08    5.86  326.0311  +19.4876
 1400  NVSS J214407+192915               3.43e+02  6.9e+01      45.00   88540 0   -1.36    6.78  326.0314  +19.4877
 1400  WB 2141+1915                      3.06e+02  6.1e+01     120.00   88540 0   -1.08    5.86  326.0233  +19.4842
 1465  [RLM94] 2141+192A                 3.05e+02  6.1e+01       4.50   88540 0   -1.11    5.96  326.0313  +19.4863
 4850  87GB 214144.6+191513              7.60e+01  1.5e+01     138.00   88540 0   -1.06    5.83  326.0217  +19.4836
 4850  BWE 2141+1915                     7.10e+01  1.4e+01     138.00   88540 0   -1.06    5.83  326.0233  +19.4842
 4850  GB6 B2141+1915                    5.70e+01  1.1e+01     108.00   88540 0   -1.36    6.78  326.0271  +19.4828
 4850  MITG J214405+1929                 5.80e+01  1.2e+01     258.00   88540 0   -1.08    5.86  326.0242  +19.4864
 4850  MITG J214410+1930                 7.40e+01  1.5e+01     258.00   88540 0   -1.06    5.83  326.0450  +19.5044

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 J2144.1+1929                 6.96e+03  1.4e+03      79.98    88540  326.0308  +19.4869
   178  4C +19.71                         2.50e+03  7.5e+02     690.00    88540  326.0317  +19.4817
  1400  WB 2141+1915                      3.06e+02  6.1e+01     120.00    88540  326.0233  +19.4842
  1465  [RLM94] 2141+192B                 1.63e+02  3.3e+01       4.50   -88540  326.0311  +19.4886
  4850  87GB 214144.6+191513              7.60e+01  1.5e+01     138.00    88540  326.0217  +19.4836

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