Complement to VIII/85A

Source 87GB_082540.4+253730: 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 J0828.6+2528 1.18e+03 2.4e+02 79.98 33363 0 -0.98 4.90 127.1608 +25.4738 151 7C 082539.39+253827.00 5.35e+02 1.1e+02 70.20 33363 0 -0.98 4.90 127.1612 +25.4742 365 TXS 0825+256 2.50e+02 5.0e+01 6.00 33363 0 -0.93 4.76 127.1601 +25.4754 1400 FIRST J082838.6+252827 6.05e+01 1.2e+01 5.00 33363 0 -0.95 4.79 127.1612 +25.4744 1400 NVSS J082838+252827 6.69e+01 1.3e+01 45.00 33363 0 -0.97 4.89 127.1616 +25.4742 4850 87GB 082540.4+253730 3.98e+01 8.0e+00 138.00 33363 0 -0.98 4.90 127.1654 +25.4583 4850 BWE 0825+2537 2.80e+01 6.6e+00 138.00 33363 0 -0.93 4.76 127.1562 +25.4564 4850 GB6 B0825+2537 2.00e+01 4.0e+00 108.00 33363 0 -0.98 4.90 127.1525 +25.4633
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%