Complement to VIII/85A

Source PMN_J0525-6938: 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
408 MRC 0525-696 9.29e+03 1.9e+03 120.00 19744 0 -0.66 5.69 081.2608 -69.6428 843 SUMSS J052502-693838 5.45e+03 1.1e+03 18.00 19744 0 -0.66 5.69 081.2596 -69.6441 1400 [FHW95]a LMCB0525-6941 4.21e+03 8.4e+02 912.00 19744 0 -0.66 5.69 081.3016 -69.6494 2450 [FHW95]b LMCB0525-6941 2.71e+03 5.4e+02 531.00 19744 0 -0.66 5.69 081.2525 -69.6414 2700 PKS J0525-6938 2.68e+03 5.4e+02 60.00 19744 0 -0.66 5.69 081.2604 -69.6425 4750 [FHW95]c LMCB0525-6941 2.25e+03 4.5e+02 288.00 19744 0 -0.66 5.69 081.2525 -69.6431 4850 PMN J0525-6938 1.69e+03 3.4e+02 168.00 19744 0 -0.66 5.69 081.2613 -69.6442 8550 [FHW95]d LMCB0525-6941 1.44e+03 2.9e+02 162.00 19744 0 -0.66 5.69 081.2925 -69.6419
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%