Complement to VIII/85A

Source VLSS_J1358.1+0133: 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 J1358.1+0133                 8.19e+03  1.6e+03      79.98   62295 4   -1.03    5.84  209.5454  +01.5602
  365  TXS 1355+018                      1.81e+03  3.6e+02       6.00   62295 4   -1.03    5.84  209.5452  +01.5587
 1400  NVSS J135810+013331               4.79e+02  9.6e+01      45.00   62295 4   -1.01    5.80  209.5450  +01.5586
 1400  WB 1355+0148                      3.57e+02  7.1e+01     120.00   62295 4   -1.02    5.82  209.5354  +01.5642

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  


    74  VLSS J1358.1+0133                 8.19e+03  1.6e+03      79.98    62295  209.5454  +01.5602
   178  4C +01.40                         2.00e+03  6.0e+02     690.00   -62295  209.5400  +01.5067
   365  TXS 1355+018                      1.81e+03  3.6e+02       6.00    62295  209.5452  +01.5587
   408  MRC 1355+018                      1.46e+03  2.9e+02     120.00   -62295  209.5450  +01.5578
  1400  FIRST J135810.6+013343            2.30e+02  4.6e+01       5.00   -62295  209.5445  +01.5622
  1400  FIRST J135811.0+013319            2.08e+02  4.2e+01       5.00   -62295  209.5460  +01.5553
  1400  FIRST J135814.4+013312            4.50e+00  9.0e-01       5.00   -62295  209.5603  +01.5533
  1400  FIRST J135821.3+012557            1.30e+00  3.0e-01       5.00   -62295  209.5888  +01.4326
  1400  NVSS J135748+013058               2.60e+00  5.0e-01      45.00   -62295  209.4510  +01.5163
  1400  NVSS J135810+013331               4.79e+02  9.6e+01      45.00    62295  209.5450  +01.5586
  1400  WB 1355+0148                      3.57e+02  7.1e+01     120.00    62295  209.5354  +01.5642
  2700  PKS J1358+0132                    2.10e+02  4.2e+01      60.00   -62295  209.5504  +01.5481
  4850  MITG J135814+0132                 1.15e+02  2.3e+01     258.00   -62295  209.5592  +01.5411

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