Complement to VIII/85A

Source 87GB_043027.1+323059: 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 B0430.4+3230 1.38e+02 2.8e+01 12.00 17239 0 -0.09 2.37 068.4195 +32.6198 1400 NVSS J043340+323711 1.09e+02 2.2e+01 45.00 17239 0 -0.09 2.37 068.4197 +32.6200 4850 87GB 043027.1+323059 7.50e+01 1.5e+01 138.00 17239 0 -0.16 2.55 068.4183 +32.6206 4850 BWE 0430+3231 6.50e+01 1.3e+01 138.00 17239 0 -0.18 2.57 068.4175 +32.6214 4850 GB6 B0430+3231 7.80e+01 1.6e+01 108.00 17239 0 -0.16 2.55 068.4158 +32.6219 4850 MITG J043338+3236 6.80e+01 1.4e+01 258.00 17239 0 -0.17 2.54 068.4100 +32.6142 4850 MITG J043341+3236 6.00e+01 1.2e+01 258.00 17239 0 -0.21 2.63 068.4246 +32.6089 8400 CLASS J043340.6912+323711.955 1.02e+02 2.0e+01 0.33 17239 0 -0.09 2.37 068.4195 +32.6200
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%