Complement to VIII/85A

Source WN_B0340.4+5032: 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
232 MY 034031.8+504121.5 2.10e+02 6.6e+01 150.00 15518 0 -0.53 3.71 056.0529 +50.6893 325 WN B0340.4+5032 2.42e+02 4.8e+01 12.00 15518 0 -0.51 3.67 056.0452 +50.6984 1400 NVSS J034410+504155 1.19e+02 2.4e+01 45.00 15518 0 -0.51 3.67 056.0453 +50.6987 1410 RRF 1545 1.38e+02 2.8e+01 564.00 15518 0 -0.51 3.67 056.0108 +50.7278 2700 F3R 4327 7.00e+01 2.8e+01 150.00 15518 0 -0.53 3.71 056.0375 +50.6872 4850 87GB 034031.8+503227 6.10e+01 1.2e+01 138.00 15518 0 -0.51 3.67 056.0529 +50.6981 4850 BWE 0340+5032 5.80e+01 1.2e+01 138.00 15518 0 -0.53 3.71 056.0533 +50.6989 4850 GB6 B0340+5032 5.60e+01 1.1e+01 108.00 15518 0 -0.54 3.74 056.0542 +50.6997
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%