Complement to VIII/85A

Source WISH_B1031.5-2520B: 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 J1033.8-2536 3.35e+03 6.7e+02 79.98 43839 4 -0.72 4.87 158.4650 -25.6036 325 WISH B1031.5-2520 7.94e+02 1.6e+02 18.00 43839 4 -0.51 4.21 158.4664 -25.6056 325 WISH B1031.5-2520B 6.25e+02 1.2e+02 18.00 43839 4 -0.47 4.05 158.4668 -25.6062 365 TXS 1031-253 1.04e+03 2.1e+02 6.00 43839 4 -0.72 4.87 158.4663 -25.6050 408 MRC 1031-253 8.70e+02 1.7e+02 120.00 43839 4 -0.70 4.80 158.4675 -25.6075 1400 NVSS J103351-253617 4.05e+02 8.1e+01 45.00 43839 4 -0.72 4.87 158.4662 -25.6049 2700 PKS J1033-2536 2.50e+02 5.0e+01 60.00 43839 4 -0.72 4.87 158.4708 -25.6028 4850 PMN J1033-2536 2.29e+02 4.6e+01 168.00 43839 4 -0.66 4.66 158.4613 -25.6067
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%