Complement to VIII/85A

Source FIRST_J085933.7+121633: 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
74 VLSS J0859.5+1216 1.07e+03 2.1e+02 79.98 34406 0 -0.70 4.34 134.8921 +12.2764 365 TXS 0856+124 3.79e+02 7.6e+01 6.00 34406 0 -0.73 4.42 134.8913 +12.2759 1400 FIRST J085933.7+121633 1.23e+02 2.5e+01 5.00 34406 0 -0.67 4.28 134.8907 +12.2760 1400 NVSS J085933+121634 1.27e+02 2.5e+01 45.00 34406 0 -0.67 4.28 134.8907 +12.2762 1400 WB 0856+1227 1.36e+02 2.7e+01 120.00 34406 0 -0.67 4.28 134.9054 +12.2661 4850 87GB 085653.5+122820 5.36e+01 1.1e+01 138.00 34406 0 -0.72 4.37 134.9071 +12.2769 4850 GB6 B0856+1228 5.17e+01 1.0e+01 108.00 34406 0 -0.73 4.42 134.8988 +12.2756 4850 MITG J085934+1216 6.50e+01 1.5e+01 258.00 34406 0 -0.70 4.34 134.8950 +12.2742
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%