Complement to VIII/85A

Source WISH_B1230.0-2429A: 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
74 VLSS J1232.7-2445 7.78e+03 1.6e+03 79.98 52532 0 -0.86 5.51 188.1796 -24.7637 325 WISH B1230.0-2429 2.15e+03 4.3e+02 18.00 52532 0 -0.86 5.51 188.1796 -24.7644 325 WISH B1230.0-2429A 2.06e+03 4.1e+02 18.00 52532 0 -0.86 5.51 188.1794 -24.7651 365 TXS 1230-244 2.27e+03 4.5e+02 6.00 52532 0 -0.86 5.51 188.1797 -24.7640 408 MRC 1230-244 1.93e+03 3.9e+02 120.00 52532 0 -0.86 5.51 188.1804 -24.7656 1400 NVSS J123243-244550 6.40e+02 1.3e+02 45.00 52532 0 -0.86 5.51 188.1798 -24.7641 2700 PKS J1232-2445 3.40e+02 6.8e+01 60.00 52532 0 -0.86 5.51 188.1817 -24.7608 4850 PMN J1232-2445 2.10e+02 4.2e+01 168.00 52532 0 -0.86 5.51 188.1788 -24.7614
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%