Complement to VIII/85A

Source Culb_1548+115: 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
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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
74 VLSS J1550.7+1120 9.55e+03 1.9e+03 79.98 -217909 237.6838 +11.3482 160 Culb 1548+115 5.40e+03 1.1e+03 111.00 -217909 237.6788 +11.3625 178 4C +11.50 3.90e+03 1.2e+03 690.00 -217909 237.6850 +11.3383 408 MRC 1548+114 2.34e+03 4.7e+02 120.00 -217909 237.6817 +11.3497 1400 FIRST J155043.2+112110 2.70e+02 5.4e+01 5.00 -217909 237.6801 +11.3530 2700 PKS J1550+1120 5.20e+02 1.0e+02 60.00 -217909 237.6817 +11.3461 4850 GB6 B1548+1129 5.43e+02 1.1e+02 108.00 -217909 237.6825 +11.3492 4850 MITG J155044+1121 6.41e+02 1.3e+02 258.00 -217909 237.6833 +11.3508 5000 RGB6 J1550.7+1120 4.21e+02 8.4e+01 144.00 -217909 237.6846 +11.3500

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


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