Complement to VIII/85A

Source GB6_B1920+1358: 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
365 TXS 1919+139 5.48e+02 1.1e+02 6.00 85213 6 1.44 -0.96 290.5498 +14.0580 1400 NVSS J192214+140319 4.48e+03 9.0e+02 45.00 85213 6 1.63 -1.43 290.5616 +14.0554 2695 RFS 834 1.95e+04 3.9e+03 294.00 85213 6 1.63 -1.43 290.5804 +14.0700 2700 F3R 1713 1.95e+04 3.9e+03 150.00 85213 6 1.63 -1.43 290.5804 +14.0700

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
31 NEK 49.3-0.1 6.26e+04 1.3e+04 720.00 -85213 290.5000 +14.0000 178 3CR 400 5.40e+05 1.1e+05 360.00 -85213 290.9488 +14.4983 327 WSRTGP 1919+1357 2.86e+03 5.7e+02 60.00 -85213 290.5614 +14.0517 365 TXS 1919+139 5.48e+02 1.1e+02 6.00 85213 290.5498 +14.0580 1400 GPSR 048.913-0.284 1.48e+03 3.0e+02 5.00 -85213 290.5574 +14.0504 1400 GPSR 048.930-0.280 7.90e+01 1.6e+01 5.00 -85213 290.5623 +14.0673 1400 NVSS J192148+135455 1.54e+02 3.1e+01 45.00 -85213 290.4509 +13.9153 1400 NVSS J192153+135612 3.18e+01 6.4e+00 45.00 -85213 290.4732 +13.9368 1400 NVSS J192207+135911 1.51e+01 3.0e+00 45.00 -85213 290.5312 +13.9864 1400 NVSS J192209+135723 9.73e+01 2.0e+01 45.00 -85213 290.5391 +13.9566 1400 NVSS J192212+135920 1.24e+01 2.5e+00 45.00 -85213 290.5506 +13.9889 1400 NVSS J192214+140319 4.48e+03 9.0e+02 45.00 85213 290.5616 +14.0554 1400 NVSS J192218+141009 5.63e+01 1.1e+01 45.00 -85213 290.5770 +14.1692 1400 NVSS J192222+140803 3.35e+02 6.7e+01 45.00 -85213 290.5954 +14.1344 1400 NVSS J192224+140917 3.96e+01 7.9e+00 45.00 -85213 290.6002 +14.1548 1400 NVSS J192225+140633 9.55e+02 1.9e+02 45.00 -85213 290.6077 +14.1094 1400 [WBH2005] G48.930-0.279 6.91e+01 1.4e+01 6.00 -85213 290.5622 +14.0671 2695 RFS 834 1.95e+04 3.9e+03 294.00 85213 290.5804 +14.0700 2700 [PBD2003] G048.9-00.3 2.37e+04 6.1e+03 480.00 -85213 290.5654 +14.0294 2700 [PBD2003] G049.0-00.3 1.13e+05 2.3e+04 480.00 -85213 290.6142 +14.1178 4850 GB6 B1920+1358 1.94e+04 3.9e+03 108.00 -85213 290.5838 +14.0639 4875 [ADP79] 1080 1.27e+04 2.5e+03 156.00 -85213 290.5679 +14.0639 4875 [ADP79] 1082 3.99e+03 8.0e+02 156.00 -85213 290.6083 +14.1189 8350 GPA1 049.07-0.35 2.17e+05 4.3e+04 582.00 -85213 290.6913 +14.1583 14350 GPA 049.07-0.35 2.14e+05 4.3e+04 396.00 -85213 290.6858 +14.1478

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