Complement to VIII/85A

Source 87GB_143326.2+302536: 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 1433+304                      2.57e+02  5.1e+01       6.00   60062 4   -0.11    2.70  218.8986  +30.2073
 1400  FIRST J143535.3+301224            1.96e+02  3.9e+01       5.00   60062 4   -0.10    2.64  218.8975  +30.2069
 1400  NVSS J143535+301225               2.45e+02  4.9e+01      45.00   60062 4   -0.04    2.52  218.8975  +30.2070
 1400  WB 1433+3025                      1.62e+02  3.2e+01     120.00   60062 4   -0.04    2.52  218.8988  +30.2094
 4850  87GB 143326.2+302536              1.94e+02  3.9e+01     138.00   60062 4   -0.04    2.52  218.8983  +30.2092
 4850  GB6 B1433+3025                    1.75e+02  3.5e+01     108.00   60062 4   -0.04    2.52  218.8983  +30.2067
 4850  MITG J143534+3012                 1.92e+02  3.8e+01     258.00   60062 4   -0.15    2.79  218.8938  +30.2003
 8400  CLASS J143535.4022+301224.515     3.09e+02  6.2e+01       0.33   60062 4   -0.04    2.52  218.8975  +30.2068
 8400  JVAS J1435+3012                   2.97e+02  5.9e+01       0.33   60062 4   -0.04    2.52  218.8975  +30.2068

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  


   151  7C 143326.10+302526.00            2.68e+02  5.4e+01      70.20   -60062  218.8975  +30.2064
   325  WN B1433.4+3025                   2.84e+02  5.7e+01      12.00   -60062  218.8973  +30.2075
   365  TXS 1433+304                      2.57e+02  5.1e+01       6.00    60062  218.8986  +30.2073
  1400  WB 1433+3025                      1.62e+02  3.2e+01     120.00    60062  218.8988  +30.2094
  4850  BWE 1433+3025                     1.91e+02  3.8e+01     138.00   -60062  218.8988  +30.2094
  4850  MITG J143534+3012                 1.92e+02  3.8e+01     258.00    60062  218.8938  +30.2003
  8400  CLASS J143535.4022+301224.515     3.09e+02  6.2e+01       0.33    60062  218.8975  +30.2068

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