Complement to VIII/85A

Source VLSS_J0501.7+0224: 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 J0501.7+0224                 7.80e+02  1.6e+02      79.98   18237 7   -0.46    3.75  075.4433  +02.4060
  611  NAIC 0459+023                     3.68e+02  7.4e+01     756.00   18237 7   -0.46    3.75  075.4429  +02.4008
 1400  NVSS J050145+022427               1.66e+02  3.3e+01      45.00   18237 7   -0.51    3.84  075.4378  +02.4076
 1400  WB 0459+0219                      2.01e+02  4.0e+01     120.00   18237 7   -0.46    3.75  075.4383  +02.3967
 4775  NAICGB 0459+023                   9.40e+01  1.9e+01     168.00   18237 7   -0.46    3.75  075.4442  +02.3986
 4850  87GB 045908.8+021933              1.39e+02  2.8e+01     138.00   18237 7   -0.46    3.75  075.4383  +02.3972
 4850  BWE 0459+0219                     1.04e+02  2.1e+01     138.00   18237 7   -0.65    4.35  075.4383  +02.3967
 4850  GB6 B0459+0219                    1.15e+02  2.3e+01     108.00   18237 7   -0.46    3.75  075.4392  +02.4031
 4850  MITG J050143+0225                 1.30e+02  2.6e+01     258.00   18237 7   -0.46    3.75  075.4300  +02.4228
 4850  PMN J0501+0224                    1.18e+02  2.4e+01     168.00   18237 7   -0.46    3.75  075.4387  +02.4094

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  


   611  NAIC 0459+023                     3.68e+02  7.4e+01     756.00    18237  075.4429  +02.4008
  1400  NVSS J050135+022759               2.40e+00  5.0e-01      45.00   -18237  075.3975  +02.4666
  4775  NAICGB 0459+023                   9.40e+01  1.9e+01     168.00    18237  075.4442  +02.3986
  4850  MITG J050143+0225                 1.30e+02  2.6e+01     258.00    18237  075.4300  +02.4228
  4850  PMN J0501+0224                    1.18e+02  2.4e+01     168.00    18237  075.4387  +02.4094
  8400  CLASS J050149.5989+022435.628     2.48e+01  5.0e+00       0.33   -18237  075.4566  +02.4099

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