Complement to VIII/85A

Source 6C_160448+630550: 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
38 8C 160446+630542 3.70e+03 7.4e+02 270.00 71995 0 -1.16 5.40 241.3542 +62.9611 74 VLSS J1605.4+6257 1.69e+03 3.4e+02 79.98 71995 0 -1.16 5.40 241.3596 +62.9614 151 6C 160448+630550 1.01e+03 2.0e+02 252.00 71995 0 -1.16 5.40 241.3621 +62.9636 151 7C 160447.50+630542.00 8.96e+02 1.8e+02 70.20 71995 0 -1.16 5.40 241.3587 +62.9611 232 MY 160452.2+625658.7 3.80e+02 7.6e+01 150.00 71995 0 -1.17 5.45 241.3787 +62.9496 325 WN B1604.7+6305 3.75e+02 7.5e+01 12.00 71995 0 -1.17 5.45 241.3591 +62.9611 1400 FIRST J160526.4+625740 5.79e+01 1.2e+01 5.00 71995 0 -1.17 5.45 241.3602 +62.9611 1400 NVSS J160526+625739 5.65e+01 1.1e+01 45.00 71995 0 -1.16 5.40 241.3596 +62.9610
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%