Complement to VIII/104

Source ATPMN8_J011218.92-663445: 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 1 column 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/104/spectra
Post annotation
SPECFIND V3.0 Catalog of radio continuum spectra (Stein+, 2021) [ReadMe+ftp]
The parameters of the radio spectra[image] (1658207 rows)
img(gal)
start AladinLite

nu Name S(nu) e beam Seq a b RAJ2000 DEJ2000 MHz mJy mJy arcsec [mJy] deg deg
200 GLEAM J011219-663446 6.39e+02 1.3e+02 120.0000 3820 -0.23 3.34 018.0798 -66.5797 843 SUMSS J011219-663445 4.74e+02 9.5e+01 18.0000 3820 -0.23 3.34 018.0792 -66.5794 2307 SPASS J011221-663438 3.20e+02 6.4e+01 645.0000 3820 -0.23 3.34 018.0898 -66.5773 2700 PKS J0112-6634 3.40e+02 6.8e+01 60.0000 3820 -0.23 3.34 018.0783 -66.5783 4800 ATPMN5 J011218.92-663445 3.68e+02 7.4e+01 1.8000 3820 -0.17 3.17 018.0788 -66.5792 4850 PMN J0112-6634 3.07e+02 6.1e+01 168.0000 3820 -0.23 3.34 018.0754 -66.5808 8400 ATPMN8 J011218.92-663445 4.30e+02 8.6e+01 1.2000 3820 -0.13 3.02 018.0788 -66.5792 8400 CRATES J011218-663451 3.21e+02 6.4e+01 6.0000 3820 -0.23 3.34 018.0792 -66.5793
VIII/104/waste
Post annotation
SPECFIND V3.0 Catalog of radio continuum spectra (Stein+, 2021) [ReadMe+ftp]
Source parameters based on positional cross-id[spectrum] (3570814 rows)
img(gal)
start AladinLite
No object found

Note: For the spectrum finding algorithm, the errors have been increased by 50%