Complement to VIII/85A

Source PKS_J1651+0129: 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 J165103+012923               7.14e+02  1.4e+02      45.00   73021 4   -0.03    2.94  252.7654  +01.4898
 1400  WB 1648+0134                      5.82e+02  1.2e+02     120.00   73021 4    0.11    2.43  252.7729  +01.4933
 1465  [P82] 1648+015                    7.20e+02  1.4e+02      25.80   73021 4   -0.01    2.87  252.7650  +01.4898
 2700  PKS J1651+0129                    7.80e+02  1.6e+02      60.00   73021 4   -0.03    2.94  252.7650  +01.4897
 4850  GB6 B1648+0134                    5.76e+02  1.2e+02     108.00   73021 4   -0.03    2.94  252.7621  +01.4906
 4850  MITG J165104+0129                 6.65e+02  1.3e+02     258.00   73021 4   -0.03    2.94  252.7696  +01.4878
 4850  PMN J1651+0129                    7.09e+02  1.4e+02     168.00   73021 4   -0.03    2.94  252.7683  +01.4897
 4885  [P82a] 1648+015                   7.20e+02  1.4e+02       6.00   73021 4   -0.03    2.94  252.7650  +01.4898
 8400  CLASS J165103.6612+012923.454     6.64e+02  1.3e+02       0.33   73021 4   -0.04    2.98  252.7652  +01.4898
 8400  JVAS J1651+0129                   6.80e+02  1.4e+02       0.33   73021 4   -0.03    2.94  252.7652  +01.4898

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 J165103+012923               7.14e+02  1.4e+02      45.00    73021  252.7654  +01.4898
  1400  WB 1648+0134                      5.82e+02  1.2e+02     120.00    73021  252.7729  +01.4933
  2700  PKS J1651+0129                    7.80e+02  1.6e+02      60.00    73021  252.7650  +01.4897
  4850  BWE 1648+0134                     4.57e+02  9.1e+01     138.00   -73021  252.7729  +01.4933
  4885  [P82a] 1648+015                   7.20e+02  1.4e+02       6.00    73021  252.7650  +01.4898
  8400  JVAS J1651+0129                   6.80e+02  1.4e+02       0.33    73021  252.7652  +01.4898

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