Complement to VIII/85A

Source 87GB_013721.9+642610: 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  


  365  TXS 0137+644                      6.31e+02  1.3e+02       6.00    3567 4   -0.64    4.44  025.2437  +64.6846
 1400  NVSS J014058+644103               3.12e+02  6.2e+01      45.00    3567 4   -0.64    4.44  025.2434  +64.6842
 1400  WB 0137+6426                      2.93e+02  5.9e+01     120.00    3567 4   -0.67    4.52  025.2263  +64.6883
 1410  RRF 1282                          2.54e+02  5.1e+01     564.00    3567 4   -0.64    4.44  025.2741  +64.6783
 2700  F3R 3833                          1.90e+02  3.8e+01     150.00    3567 4   -0.64    4.44  025.2625  +64.6781
 4850  87GB 013721.9+642610              1.21e+02  2.4e+01     138.00    3567 4   -0.64    4.44  025.2271  +64.6886
 4850  BWE 0137+6426                     9.70e+01  1.9e+01     138.00    3567 4   -0.75    4.76  025.2263  +64.6883
 4850  GB6 B0137+6426                    1.07e+02  2.1e+01     108.00    3567 4   -0.70    4.61  025.2321  +64.6889
 4890  KR 177                            1.00e+02  2.0e+01       3.96    3567 4   -0.64    4.44  025.2437  +64.6845

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  


   325  WN B0137.4+6425                   4.27e+02  8.5e+01      12.00    -3567  025.2432  +64.6848
   365  TXS 0137+644                      6.31e+02  1.3e+02       6.00     3567  025.2437  +64.6846
  1400  WB 0137+6426                      2.93e+02  5.9e+01     120.00     3567  025.2263  +64.6883
  1410  RRF 1282                          2.54e+02  5.1e+01     564.00     3567  025.2741  +64.6783
  2700  F3R 3833                          1.90e+02  3.8e+01     150.00     3567  025.2625  +64.6781
  4850  87GB 013721.9+642610              1.21e+02  2.4e+01     138.00     3567  025.2271  +64.6886
  4890  KR 177                            1.00e+02  2.0e+01       3.96     3567  025.2437  +64.6845

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