Complement to VIII/104

Source ATPMN5_J060425.17-422530: points from spectra and waste tables

  Postscript Figure Additional frequencies and fluxes in ν and S Data as a Table  
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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
150 TGSSADR J060425.0-422531 1.68e+02 3.4e+01 25.0020 80333 0.20 1.79 091.1043 -42.4253 843 SUMSS J060425-422530 2.45e+02 4.9e+01 18.0000 80333 0.20 1.79 091.1042 -42.4252 2307 SPASS J060424-422540 2.23e+02 4.5e+01 645.0000 80333 0.20 1.79 091.1039 -42.4280 2700 PKS J0604-4225 3.50e+02 7.0e+01 60.0000 80333 0.20 1.79 091.1046 -42.4250 4800 ATPMN5 J060425.17-422530 5.60e+02 1.1e+02 1.8000 80333 0.32 1.54 091.1049 -42.4250 4850 PMN J0604-4225 3.36e+02 6.7e+01 168.0000 80333 0.20 1.79 091.0933 -42.4258 8400 ATPMN8 J060425.17-422530 6.03e+02 1.2e+02 1.2000 80333 0.25 1.68 091.1049 -42.4250 8400 CRATES J060422-422533 5.39e+02 1.1e+02 6.0000 80333 0.25 1.67 091.1049 -42.4250
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%