Complement to VIII/85A

Source VLSS_J2348.6+5043: 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 J2348.6+5043                 7.10e+03  1.4e+03      79.98   95168 5   -0.68    5.12  357.1538  +50.7253
  178  4C +50.59                         3.30e+03  9.9e+02     690.00   95168 5   -0.68    5.12  357.1508  +50.6550
  325  WN B2346.1+5026                   2.77e+03  5.5e+02      12.00   95168 5   -0.68    5.12  357.1503  +50.7260
  365  TXS 2346+504                      2.40e+03  4.8e+02       6.00   95168 5   -0.68    5.12  357.1504  +50.7258
 1400  NVSS J234836+504332               9.48e+02  1.9e+02      45.00   95168 5   -0.68    5.12  357.1502  +50.7258
 1400  WB 2346+5026                      9.81e+02  2.0e+02     120.00   95168 5   -0.68    5.12  357.1475  +50.7239
 4850  87GB 234606.0+502646              4.12e+02  8.2e+01     138.00   95168 5   -0.68    5.12  357.1471  +50.7239
 4850  BWE 2346+5026                     4.10e+02  8.2e+01     138.00   95168 5   -0.68    5.12  357.1475  +50.7239
 4850  GB6 B2346+5026                    3.85e+02  7.7e+01     108.00   95168 5   -0.68    5.12  357.1488  +50.7253
 4850  MITG J234828+5042                 3.34e+02  6.7e+01     258.00   95168 5   -0.68    5.12  357.1192  +50.7044

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  


   178  4C +50.59                         3.30e+03  9.9e+02     690.00    95168  357.1508  +50.6550
   232  MY 234600.4+504442.3              7.29e+03  1.5e+03     150.00   -95168  357.1233  +50.7451
  1400  NVSS J234841+504237               7.30e+00  1.5e+00      45.00   -95168  357.1747  +50.7103
  4850  87GB 234606.0+502646              4.12e+02  8.2e+01     138.00    95168  357.1471  +50.7239
  4850  GB6 B2346+5026                    3.85e+02  7.7e+01     108.00    95168  357.1488  +50.7253
  4850  MITG J234828+5042                 3.34e+02  6.7e+01     258.00    95168  357.1192  +50.7044

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