Complement to VIII/85A

Source WN_B1145.6+7844: 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
38 8C 114542+784336 2.70e+03 5.4e+02 270.00 104201 0 -0.55 4.30 177.1417 +78.4489 74 VLSS J1148.4+7827 1.60e+03 3.2e+02 79.98 104201 0 -0.55 4.30 177.1246 +78.4572 151 6C 114536+784354 1.45e+03 2.9e+02 252.00 104201 0 -0.55 4.30 177.1192 +78.4539 151 7C 114536.20+784401.00 1.41e+03 2.8e+02 70.20 104201 0 -0.55 4.30 177.1192 +78.4556 232 MY 114538.2+782707.1 1.00e+03 2.0e+02 150.00 104201 0 -0.55 4.30 177.1275 +78.4520 325 WN B1145.6+7844 9.70e+02 1.9e+02 12.00 104201 0 -0.55 4.30 177.1213 +78.4556 1400 NVSS J114829+782721 4.19e+02 8.4e+01 45.00 104201 0 -0.52 4.25 177.1216 +78.4560 1400 WB 1145+7843 3.75e+02 7.5e+01 120.00 104201 0 -0.55 4.30 177.0888 +78.4544
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%