Complement to VIII/85A

Source MITG_J223400+1008: 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
365 TXS 2231+098 5.87e+02 1.2e+02 6.00 107253 4 -0.23 3.35 338.4935 +10.1479 1400 NVSS J223358+100852 3.60e+02 7.2e+01 45.00 107253 4 -0.23 3.35 338.4935 +10.1478 1400 WB 2231+0953 4.54e+02 9.1e+01 120.00 107253 4 -0.23 3.35 338.4908 +10.1497 4850 87GB 223128.4+095325 3.21e+02 6.4e+01 138.00 107253 4 -0.23 3.35 338.4908 +10.1486 4850 BWE 2231+0953 2.74e+02 5.5e+01 138.00 107253 4 -0.23 3.35 338.4908 +10.1497 4850 GB6 B2231+0953 3.26e+02 6.5e+01 108.00 107253 4 -0.23 3.35 338.4942 +10.1486 4850 MITG J223400+1008 4.25e+02 8.5e+01 258.00 107253 4 -0.23 3.35 338.5029 +10.1397 8400 JVAS J2233+1008 2.87e+02 5.7e+01 0.33 107253 4 -0.23 3.35 338.4935 +10.1478
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%