Complement to VIII/85A

Source PMN_J1938+0942: 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
1400 NVSS J193843+094220 3.21e+02 6.4e+01 45.00 82589 4 -0.36 3.63 294.6817 +09.7056 1400 WB 1936+0935 2.91e+02 5.8e+01 120.00 82589 4 -0.36 3.63 294.6837 +09.7072 4850 87GB 193620.6+093530 2.42e+02 4.8e+01 138.00 82589 4 -0.43 3.87 294.6833 +09.7067 4850 BWE 1936+0935 1.97e+02 3.9e+01 138.00 82589 4 -0.38 3.65 294.6837 +09.7072 4850 GB6 B1936+0935 2.60e+02 5.2e+01 108.00 82589 4 -0.43 3.87 294.6821 +09.7053 4850 PMN J1938+0942 2.06e+02 4.1e+01 168.00 82589 4 -0.43 3.87 294.6792 +09.7081 8400 CLASS J193843.6015+094220.091 1.48e+02 3.0e+01 0.33 82589 4 -0.36 3.63 294.6817 +09.7056 8400 JVAS J1938+0942 1.55e+02 3.1e+01 0.33 82589 4 -0.36 3.63 294.6817 +09.7056
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%