Complement to VIII/85A

Source WN_B1426.5+4253: 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 B1426.5+4253 6.40e+01 1.3e+01 12.00 59843 0 -0.26 2.46 217.1350 +42.6724 1400 FIRST J142832.6+424021 4.36e+01 8.7e+00 5.00 59843 0 -0.26 2.46 217.1359 +42.6726 1400 NVSS J142832+424022 5.80e+01 1.2e+01 45.00 59843 0 -0.26 2.46 217.1356 +42.6729 4850 87GB 142634.5+425353 4.37e+01 8.7e+00 138.00 59843 0 -0.26 2.46 217.1300 +42.6756 4850 BWE 1426+4253 3.50e+01 7.0e+00 138.00 59843 0 -0.26 2.46 217.1304 +42.6769 4850 GB6 B1426+4253 3.50e+01 7.0e+00 108.00 59843 0 -0.26 2.46 217.1267 +42.6772 4885 RGB 1428+426 3.10e+01 6.2e+00 4.02 59843 0 -0.26 2.46 217.1359 +42.6725 8400 CLASS J142832.6071+424021.056 2.74e+01 5.5e+00 0.33 59843 0 -0.26 2.46 217.1358 +42.6725
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%