Complement to VIII/85A

Source 87GB_152959.0+302636: 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 B1529.9+3026 6.00e+01 1.2e+01 12.00 66702 0 -0.10 2.03 233.0090 +30.2738 1400 FIRST J153202.2+301628 6.12e+01 1.2e+01 5.00 66702 0 -0.10 2.02 233.0093 +30.2747 1400 NVSS J153202+301629 5.23e+01 1.0e+01 45.00 66702 0 -0.10 2.02 233.0095 +30.2748 4850 87GB 152959.0+302636 5.50e+01 1.1e+01 138.00 66702 0 -0.10 2.03 233.0067 +30.2750 4850 BWE 1529+3026 5.30e+01 1.1e+01 138.00 66702 0 -0.10 2.03 233.0054 +30.2747 4850 GB6 B1529+3026 4.20e+01 8.4e+00 108.00 66702 0 -0.10 2.03 233.0096 +30.2775 4885 RGB 1532+302 4.20e+01 8.4e+00 4.02 66702 0 -0.10 2.03 233.0092 +30.2747 8400 CLASS J153202.2298+301628.844 4.38e+01 8.8e+00 0.33 66702 0 -0.10 2.03 233.0092 +30.2747
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%