Complement to VIII/85A

Source NVSS_J125834+003833: points from spectra and waste tables

  Postscript Figure Additional frequencies and fluxes in ν and S Data as a Table  
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VIII/85A/spectra
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SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009) [ReadMe+ftp]
The parameters of the radio spectra[image][spectrum] (631736 rows)
img(gal)
start AladinLite
No object foundThe 1 column 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/waste
Post annotation
SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009) [ReadMe+ftp]
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 J125834.9+003832 6.47e+01 1.3e+01 5.00 -197061 194.6455 +00.6423 1400 FIRST J125834.9+003901 2.40e+00 5.0e-01 5.00 -197061 194.6457 +00.6504 1400 FIRST J125836.2+003950 2.00e+00 4.0e-01 5.00 -197061 194.6510 +00.6639 1400 FIRST J125841.4+003540 9.00e-01 2.0e-01 5.00 -197061 194.6725 +00.5946 1400 FIRST J125848.6+003746 2.30e+00 5.0e-01 5.00 -197061 194.7027 +00.6296 1400 FIRST J125848.9+003806 1.42e+01 2.8e+00 5.00 -197061 194.7040 +00.6351 1400 NVSS J125834+003833 7.83e+01 1.6e+01 45.00 -197061 194.6455 +00.6425 1400 NVSS J125848+003806 1.96e+01 3.9e+00 45.00 -197061 194.7038 +00.6350 4850 PMN J1258+0038 1.67e+02 3.3e+01 168.00 -197061 194.6483 +00.6433 8400 CLASS J125834.9108+003832.115 6.77e+01 1.4e+01 0.33 -197061 194.6455 +00.6423

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