Complement to VIII/85A

Source GPSR_087.881+0.093: 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]
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
325 WN B2101.3+4637 1.38e+02 2.8e+01 12.00 91965 0 -0.92 4.46 315.7817 +46.8282 327 WSRTGP 2101+4637 1.26e+02 2.5e+01 60.00 91965 0 -1.67 6.34 315.7820 +46.8300 408 B3 2101+466 1.00e+02 2.0e+01 84.00 91965 0 -1.67 6.34 315.7796 +46.8361 1400 GPSR 087.881+0.093 1.20e+01 2.4e+00 5.00 91965 0 -1.67 6.34 315.7802 +46.8292 1400 GPSR 087.882+0.092 1.70e+01 3.4e+00 5.00 91965 0 -1.43 5.74 315.7829 +46.8296 1400 NVSS J210307+464945 4.37e+01 8.7e+00 45.00 91965 0 -0.92 4.46 315.7823 +46.8294 1400 [WBH2005] G87.880+0.094 1.15e+01 2.3e+00 6.00 91965 0 -1.70 6.41 315.7802 +46.8294 1400 [WBH2005] G87.882+0.092 2.04e+01 4.1e+00 6.00 91965 0 -1.43 5.74 315.7832 +46.8296
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
No object found

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