Complement to VIII/85A

Source NVSS_J153447+371554: 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 B1532.8+3725 2.00e+01 4.0e+00 12.00 66787 0 0.06 1.14 233.6931 +37.2646 1400 FIRST J153447.2+371554 2.21e+01 4.4e+00 5.00 66787 0 0.06 1.14 233.6967 +37.2652 1400 NVSS J153447+371554 2.20e+01 4.4e+00 45.00 66787 0 0.06 1.14 233.6972 +37.2650 4850 87GB 153254.4+372523 3.20e+01 6.4e+00 138.00 66787 0 0.06 1.14 233.6967 +37.2575 4850 BWE 1532+3725 2.90e+01 6.7e+00 138.00 66787 0 0.06 1.14 233.6983 +37.2556 4850 GB6 B1532+3725 2.40e+01 4.8e+00 108.00 66787 0 0.06 1.14 233.6942 +37.2581 4885 RGB 1534+372 2.40e+01 4.8e+00 4.02 66787 0 0.06 1.14 233.6967 +37.2651 8400 CLASS J153447.2066+371554.615 1.93e+01 3.9e+00 0.33 66787 0 0.06 1.14 233.6967 +37.2652
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%


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