Complement to VIII/85A

Source WN_B1359.4+3625: 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 B1359.4+3625 7.30e+01 1.5e+01 12.00 58964 0 0.00 1.86 210.4115 +36.1896 1400 FIRST J140138.7+361122 8.30e+01 1.7e+01 5.00 58964 0 0.00 1.86 210.4114 +36.1895 1400 NVSS J140138+361121 7.24e+01 1.4e+01 45.00 58964 0 -0.01 1.88 210.4115 +36.1894 4850 87GB 135932.3+362554 7.26e+01 1.5e+01 138.00 58964 0 0.00 1.86 210.4225 +36.1911 4850 BWE 1359+3625 5.90e+01 1.2e+01 138.00 58964 0 0.00 1.86 210.4217 +36.1906 4850 GB6 B1359+3625 6.90e+01 1.4e+01 108.00 58964 0 0.00 1.86 210.4171 +36.1883 4850 MITG J140141+3611 6.20e+01 1.2e+01 258.00 58964 0 0.00 1.86 210.4212 +36.1889 8400 CLASS J140138.7327+361121.908 7.36e+01 1.5e+01 0.33 58964 0 0.00 1.86 210.4114 +36.1894
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%