Complement to VIII/104

Source VLSSr_J063521.0-262040: 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
74 VLSSr J063521.0-262040 6.20e+02 1.2e+02 75.0000 99603 -0.13 3.04 098.8377 -26.3445 150 TGSSADR J063519.8-262046 3.26e+02 6.5e+01 25.0020 99603 0.10 2.26 098.8328 -26.3463 200 GLEAM J063520-262043 3.13e+02 6.3e+01 120.0000 99603 0.10 2.26 098.8337 -26.3455 1400 NVSS J063520-262048 3.46e+02 6.9e+01 45.0000 99603 0.10 2.26 098.8335 -26.3469 2307 SPASS J063519-262036 4.02e+02 8.0e+01 645.0000 99603 0.10 2.26 098.8323 -26.3434 4850 PMN J0635-2620 3.57e+02 7.1e+01 168.0000 99603 0.10 2.26 098.8383 -26.3467 8400 CRATES J063521-262048 2.46e+02 4.9e+01 6.0000 99603 -0.05 2.66 098.8371 -26.3444 22000 K-RFC J0635-2620 5.40e+02 1.5e+02 126.0000 99603 0.10 2.26 098.8371 -26.3444
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%