Complement to VIII/85A

Source GPSR5_359.952-0.046: 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="

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
No object foundThe 1 column 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/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

nu Name S(nu) e beam Seq RAJ2000 DEJ2000 MHz mJy mJy arcsec deg deg
160 Culb 1742-290 1.09e+05 2.2e+04 111.00 -234324 266.4379 -29.0194 1400 GPSR 359.944-0.046 7.85e+02 1.6e+02 5.00 -234324 266.4164 -29.0074 1410 RRF 10 4.48e+05 9.0e+04 564.00 -234324 266.4175 -28.9867 2695 RFS 1211 2.45e+05 4.9e+04 294.00 -234324 266.4304 -29.0067 2700 [PBD2003] G359.9-00.0 3.60e+05 7.2e+04 480.00 -234324 266.3450 -29.0228 4850 PMN J1746-2848 2.71e+04 5.4e+03 168.00 -234324 266.5496 -28.8089 4875 [ADP79] 47 1.98e+05 4.0e+04 156.00 -234324 266.4258 -29.0117 4900 GPSR5 359.952-0.046 2.78e+03 5.6e+02 4.02 -234324 266.4168 -29.0078 8350 GPA1 000.02-0.05 5.23e+05 1.0e+05 582.00 -234324 266.4633 -28.9472 8350 GPA1 359.99-0.02 1.97e+05 3.9e+04 582.00 -234324 266.4220 -28.9575

Note: For the spectrum finding algorithm, the errors have been increased by 50%