Complement to VIII/85A

Source MY_053701.4+555006.2: 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  


  151  6C 053703+554917                  3.10e+02  6.2e+01     252.00   22899 1   -0.18    2.83  085.3142  +55.8467
  232  MY 053701.4+555006.2              2.90e+02  7.2e+01     150.00   22899 1   -0.14    2.79  085.3046  +55.8351
  325  WN B0537.0+5549                   2.32e+02  4.6e+01      12.00   22899 1   -0.35    3.26  085.3110  +55.8446
 1400  NVSS J054114+555043               1.41e+02  2.8e+01      45.00   22899 1   -0.14    2.79  085.3114  +55.8454
 1400  WB 0537+5549                      1.77e+02  3.5e+01     120.00   22899 1   -0.14    2.79  085.3088  +55.8500
 4850  87GB 053702.2+554928              1.83e+02  3.7e+01     138.00   22899 1   -0.14    2.79  085.3083  +55.8497
 4850  BWE 0537+5549                     1.79e+02  3.6e+01     138.00   22899 1   -0.16    2.84  085.3088  +55.8500
 4850  GB6 B0537+5549                    1.92e+02  3.8e+01     108.00   22899 1   -0.14    2.79  085.3088  +55.8469
 8400  CLASS J054114.7577+555043.555     1.76e+02  3.5e+01       0.33   22899 1   -0.14    2.79  085.3115  +55.8454

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  6C 053703+554917                  3.10e+02  6.2e+01     252.00    22899  085.3142  +55.8467
   232  MY 053701.4+555006.2              2.90e+02  7.2e+01     150.00    22899  085.3046  +55.8351
   325  WN B0537.0+5549                   2.32e+02  4.6e+01      12.00    22899  085.3110  +55.8446
  1400  NVSS J054113+554934               1.41e+01  2.8e+00      45.00   -22899  085.3050  +55.8264
  1400  NVSS J054114+555043               1.41e+02  2.8e+01      45.00    22899  085.3114  +55.8454
  4850  GB6 B0537+5549                    1.92e+02  3.8e+01     108.00    22899  085.3088  +55.8469
  8400  CLASS J054114.7577+555043.555     1.76e+02  3.5e+01       0.33    22899  085.3115  +55.8454

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