Complement to VIII/85A

Source NVSS_J141509+083206: 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  FIRST J141509.9+083205            1.57e+02  3.1e+01       5.00   61619 0    0.69   -0.20  213.7913  +08.5348
 1400  NVSS J141509+083206               8.92e+01  1.8e+01      45.00   61619 0    0.69   -0.20  213.7913  +08.5352
 1400  WB 1412+0845                      2.00e+02  4.0e+01     120.00   61619 0    0.69   -0.20  213.7883  +08.5278
 4850  MITG J141511+0832                 2.61e+02  5.2e+01     258.00   61619 0    0.69   -0.20  213.7988  +08.5367
 8400  CLASS J141509.9185+083205.378     2.60e+02  5.2e+01       0.33   61619 0    0.41    0.91  213.7913  +08.5348

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  FIRST J141458.1+083330            2.30e+00  5.0e-01       5.00   -61619  213.7424  +08.5585
  1400  FIRST J141500.3+083432            1.30e+00  3.0e-01       5.00   -61619  213.7516  +08.5758
  1400  FIRST J141501.7+082806            1.50e+00  3.0e-01       5.00   -61619  213.7572  +08.4685
  1400  FIRST J141509.9+083205            1.57e+02  3.1e+01       5.00    61619  213.7913  +08.5348
  1400  NVSS J141458+083335               3.60e+00  7.0e-01      45.00   -61619  213.7430  +08.5599
  1400  NVSS J141509+083206               8.92e+01  1.8e+01      45.00    61619  213.7913  +08.5352
  1400  WB 1412+0845                      2.00e+02  4.0e+01     120.00    61619  213.7883  +08.5278
  4850  87GB 141240.9+084531              9.88e+01  2.0e+01     138.00   -61619  213.7879  +08.5264
  4850  BWE 1412+0845                     7.80e+01  1.6e+01     138.00   -61619  213.7883  +08.5278
  4850  GB6 B1412+0846                    7.80e+01  1.6e+01     108.00   -61619  213.7912  +08.5347
  4850  PMN J1415+0832                    2.09e+02  4.2e+01     168.00   -61619  213.7892  +08.5369
  8400  CLASS J141509.9185+083205.378     2.60e+02  5.2e+01       0.33    61619  213.7913  +08.5348

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