Complement to VIII/85A

Source GB6_B1423+3417: 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 B1424.0+3417 4.00e+01 8.0e+00 12.00 59770 0 -0.13 1.93 216.5312 +34.0751 1400 FIRST J142607.7+340426 3.57e+01 7.1e+00 5.00 59770 0 -0.13 1.93 216.5322 +34.0740 1400 NVSS J142607+340426 3.46e+01 6.9e+00 45.00 59770 0 -0.13 1.93 216.5317 +34.0740 4850 87GB 142357.8+341753 4.11e+01 8.2e+00 138.00 59770 0 -0.13 1.95 216.5196 +34.0736 4850 BWE 1423+3417 3.50e+01 7.0e+00 138.00 59770 0 -0.13 1.93 216.5204 +34.0747 4850 GB6 B1423+3417 3.36e+01 6.7e+00 108.00 59770 0 -0.13 1.93 216.5250 +34.0742 4885 RGB 1426+340 2.80e+01 5.6e+00 4.02 59770 0 -0.13 1.93 216.5321 +34.0739 8400 CLASS J142607.7146+340426.309 2.51e+01 5.0e+00 0.33 59770 0 -0.13 1.93 216.5321 +34.0740
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%