Complement to VIII/104

Source PKS_J0738-6735: 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 J073856-673550 5.03e+02 1.0e+02 120.0000 113933 -0.10 2.97 114.7359 -67.5973 843 SUMSS J073856-673551 5.45e+02 1.1e+02 18.0000 113933 -0.16 3.21 114.7350 -67.5977 2307 SPASS J073901-673545 4.84e+02 9.7e+01 645.0000 113933 -0.16 3.21 114.7574 -67.5961 2700 PKS J0738-6735 4.50e+02 9.0e+01 60.0000 113933 -0.16 3.21 114.7358 -67.5969 4800 ATPMN5 J073856.49-673550 3.34e+02 6.7e+01 1.8000 113933 -0.06 2.85 114.7353 -67.5975 4850 PMN J0738-6735 3.76e+02 7.5e+01 168.0000 113933 -0.16 3.21 114.7267 -67.5958 8400 ATPMN8 J073856.49-673550 3.96e+02 7.9e+01 1.2000 113933 -0.06 2.85 114.7353 -67.5975 8400 CRATES J073854-673545 3.76e+02 7.5e+01 6.0000 113933 -0.16 3.21 114.7353 -67.5976
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%