Complement to VIII/85A

Source JVAS_J0614+510: 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
325 WN B0610.8+5103 1.97e+02 3.9e+01 12.00 24042 4 -0.06 2.45 093.7049 +51.0372 1400 NVSS J061449+510213 1.65e+02 3.3e+01 45.00 24042 4 -0.06 2.45 093.7045 +51.0370 1400 WB 0610+5103 1.56e+02 3.1e+01 120.00 24042 4 0.00 2.29 093.6992 +51.0406 4850 87GB 061051.6+510321 2.02e+02 4.0e+01 138.00 24042 4 -0.06 2.45 093.6992 +51.0403 4850 BWE 0610+5103 1.98e+02 4.0e+01 138.00 24042 4 -0.06 2.45 093.6992 +51.0406 4850 GB6 B0610+5103 1.98e+02 4.0e+01 108.00 24042 4 -0.06 2.45 093.7029 +51.0397 8400 CLASS J061449.1578+510213.112 1.62e+02 3.2e+01 0.33 24042 4 -0.06 2.45 093.7048 +51.0370 8400 JVAS J0614+510 1.64e+02 3.3e+01 0.33 24042 4 -0.06 2.44 093.7048 +51.0370
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%