Complement to VIII/85A

Source F3R_2722: 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 204043.7+425729.7 1.33e+04 2.7e+03 150.00 86556 0 -0.02 4.18 310.6263 +42.9583 325 WN B2040.8+4246 1.27e+04 2.5e+03 12.00 86556 0 -0.02 4.18 310.6454 +42.9509 1410 RRF 747 1.62e+04 3.2e+03 564.00 86556 0 -0.02 4.18 310.6467 +42.9372 2700 F3R 2722 1.70e+04 3.4e+03 150.00 86556 0 -0.02 4.18 310.6458 +42.9439 4850 GB6 B2040+4242 4.16e+03 8.3e+02 108.00 86556 0 -0.38 5.03 310.6250 +42.8953 4850 GB6 B2040+4246 1.09e+04 2.2e+03 108.00 86556 0 -0.02 4.18 310.6742 +42.9558 4850 MITG J204239+4257 3.33e+03 6.7e+02 258.00 86556 0 -0.46 5.20 310.6633 +42.9511 8350 GPA1 082.60+0.39 1.60e+04 3.2e+03 582.00 86556 0 -0.02 4.18 310.6767 +42.9600 14350 GPA 082.60+0.39 1.20e+04 2.4e+03 396.00 86556 0 -0.02 4.18 310.6358 +42.9603

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
232 MY 204043.7+425729.7 1.33e+04 2.7e+03 150.00 86556 310.6263 +42.9583 325 WN B2040.8+4246 1.27e+04 2.5e+03 12.00 86556 310.6454 +42.9509 327 WSRTGP 2041+4249 6.30e+01 1.3e+01 60.00 -86556 310.7342 +43.0133 1400 NVSS J204218+425442 9.95e+02 2.0e+02 45.00 -86556 310.5772 +42.9118 1400 NVSS J204220+425723 9.05e+02 1.8e+02 45.00 -86556 310.5848 +42.9564 1400 NVSS J204232+425634 1.20e+02 2.4e+01 45.00 -86556 310.6357 +42.9430 1400 NVSS J204232+425813 2.25e+03 4.5e+02 45.00 -86556 310.6366 +42.9704 1400 NVSS J204238+425932 1.34e+02 2.7e+01 45.00 -86556 310.6613 +42.9924 1400 NVSS J204246+425811 1.31e+03 2.6e+02 45.00 -86556 310.6942 +42.9697 1400 NVSS J204257+425554 5.59e+02 1.1e+02 45.00 -86556 310.7403 +42.9317 1410 RRF 747 1.62e+04 3.2e+03 564.00 86556 310.6467 +42.9372 2700 F3R 2722 1.70e+04 3.4e+03 150.00 86556 310.6458 +42.9439 2700 [PBD2003] G082.6+00.4 2.53e+04 5.1e+03 480.00 -86556 310.6683 +42.9683 4850 GB6 B2040+4242 4.16e+03 8.3e+02 108.00 86556 310.6250 +42.8953 4850 GB6 B2040+4246 1.09e+04 2.2e+03 108.00 86556 310.6742 +42.9558 4850 MITG J204210+4255 1.03e+03 2.1e+02 258.00 -86556 310.5446 +42.9236 4850 MITG J204239+4257 3.33e+03 6.7e+02 258.00 86556 310.6633 +42.9511 4850 MITG J204257+4258 1.07e+03 2.1e+02 258.00 -86556 310.7400 +42.9822 8350 GPA1 082.60+0.39 1.60e+04 3.2e+03 582.00 86556 310.6767 +42.9600 14350 GPA 082.60+0.39 1.20e+04 2.4e+03 396.00 86556 310.6358 +42.9603

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