Complement to VIII/85A

Source GB6_B1016+6335: 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 B1016.3+6335 1.13e+02 2.3e+01 12.00 41510 4 0.27 1.37 154.9623 +63.3342 1400 FIRST J101950.8+632001 1.18e+02 2.4e+01 5.00 41510 4 0.23 1.44 154.9621 +63.3338 1400 NVSS J101950+632002 1.09e+02 2.2e+01 45.00 41510 4 0.21 1.47 154.9621 +63.3340 4850 87GB 101619.9+633457 2.71e+02 5.4e+01 138.00 41510 4 0.27 1.37 154.9633 +63.3314 4850 BWE 1016+6334 2.65e+02 5.3e+01 138.00 41510 4 0.23 1.44 154.9642 +63.3311 4850 GB6 B1016+6335 2.37e+02 4.7e+01 108.00 41510 4 0.27 1.37 154.9596 +63.3322 8400 CLASS J101950.8733+632001.616 2.73e+02 5.5e+01 0.33 41510 4 0.27 1.37 154.9620 +63.3338 8400 JVAS J1019+633 2.68e+02 5.4e+01 0.33 41510 4 0.27 1.39 154.9620 +63.3338
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%