Complement to VIII/85A

Source VLSS_J1214.9+0311: 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
74 VLSS J1214.9+0311 1.41e+03 2.8e+02 79.98 50344 0 -0.63 4.32 183.7433 +03.1952 1400 FIRST J121458.5+031135 2.34e+02 4.7e+01 5.00 50344 0 -0.64 4.35 183.7439 +03.1933 1400 NVSS J121458+031135 2.22e+02 4.4e+01 45.00 50344 0 -0.64 4.35 183.7437 +03.1931 4850 87GB 121222.8+032740 9.70e+01 1.9e+01 138.00 50344 0 -0.63 4.32 183.7346 +03.1833 4850 BWE 1212+0327 9.40e+01 1.9e+01 138.00 50344 0 -0.63 4.32 183.7346 +03.1836 4850 GB6 B1212+0328 1.03e+02 2.1e+01 108.00 50344 0 -0.63 4.32 183.7488 +03.1906 4850 MITG J121457+0309 1.08e+02 2.2e+01 258.00 50344 0 -0.63 4.32 183.7383 +03.1511 4850 PMN J1214+0311 9.40e+01 1.9e+01 168.00 50344 0 -0.63 4.32 183.7392 +03.1956
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%