Complement to VIII/85A

Source MITG_J042653+2326: 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 WB 0423+2321 5.87e+02 1.2e+02 120.00 17005 0 -0.46 4.22 066.7288 +23.4631 4850 87GB 042354.5+232103 3.37e+02 6.7e+01 138.00 17005 0 -0.46 4.22 066.7279 +23.4625 4850 BWE 0423+2321 3.31e+02 6.6e+01 138.00 17005 0 -0.46 4.22 066.7288 +23.4631 4850 GB6 B0423+2320 3.32e+02 6.6e+01 108.00 17005 0 -0.46 4.22 066.7325 +23.4614 4850 MITG J042653+2326 3.30e+02 6.6e+01 258.00 17005 0 -0.46 4.22 066.7212 +23.4481 4850 MITG J042653+2327 3.22e+02 6.4e+01 258.00 17005 0 -0.46 4.22 066.7242 +23.4525 8400 CLASS J042655.7370+232739.670 2.70e+02 5.4e+01 0.33 17005 0 -0.46 4.22 066.7322 +23.4610 8400 JVAS J0426+2327 2.66e+02 5.3e+01 0.33 17005 0 -0.44 4.16 066.7322 +23.4610
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%