Complement to VIII/85A

Source GB6_B2104+4659: 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 210403.4+471117.3 1.60e+03 3.2e+02 150.00 87269 6 -0.88 5.22 316.4479 +47.1881 325 WN B2104.0+4659 1.36e+03 2.7e+02 12.00 87269 6 -1.03 5.66 316.4576 +47.1997 327 WSRTGP 2104+4659A 1.22e+03 2.4e+02 60.00 87269 6 -1.03 5.66 316.4579 +47.2003 365 TXS 2104+469 1.12e+03 2.2e+02 6.00 87269 6 -1.03 5.66 316.4570 +47.1999 408 B3 2104+469 9.40e+02 1.9e+02 84.00 87269 6 -1.03 5.66 316.4596 +47.2006 1400 NVSS J210549+471158 2.77e+02 5.5e+01 45.00 87269 6 -1.03 5.66 316.4579 +47.1996 1410 RRF 802 2.90e+02 5.8e+01 564.00 87269 6 -1.04 5.72 316.4437 +47.1806 2700 F3R 2853 1.40e+02 2.8e+01 150.00 87269 6 -0.88 5.22 316.4504 +47.1953 4850 87GB 210403.6+465922 6.38e+01 1.3e+01 138.00 87269 6 -1.04 5.72 316.4488 +47.1903 4850 BWE 2104+4659 4.90e+01 9.8e+00 138.00 87269 6 -1.04 5.71 316.4492 +47.1931 4850 GB6 B2104+4659 6.27e+01 1.3e+01 108.00 87269 6 -1.04 5.71 316.4554 +47.1928 4850 MITG J210551+4712 6.00e+01 1.2e+01 258.00 87269 6 -1.04 5.71 316.4650 +47.2036

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 J2105.8+4711 3.69e+03 7.4e+02 79.98 -87269 316.4592 +47.1994 232 MY 210403.4+471117.3 1.60e+03 3.2e+02 150.00 87269 316.4479 +47.1881 325 WN B2104.0+4659 1.36e+03 2.7e+02 12.00 87269 316.4576 +47.1997 327 WSRTGP 2104+4659A 1.22e+03 2.4e+02 60.00 87269 316.4579 +47.2003 365 TXS 2104+469 1.12e+03 2.2e+02 6.00 87269 316.4570 +47.1999 408 B3 2104+469 9.40e+02 1.9e+02 84.00 87269 316.4596 +47.2006 1400 GPSR 088.458-0.003 3.50e+01 7.0e+00 5.00 -87269 316.4513 +47.1947 1400 GPSR 088.458-0.007 4.70e+01 9.4e+00 5.00 -87269 316.4558 +47.1921 1400 GPSR 088.468-0.001 1.39e+02 2.8e+01 5.00 -87269 316.4590 +47.2030 1400 NVSS J210549+471158 2.77e+02 5.5e+01 45.00 87269 316.4579 +47.1996 1400 [WBH2005] G88.458-0.003 3.60e+01 7.2e+00 6.00 -87269 316.4517 +47.1946 1400 [WBH2005] G88.458-0.007 5.48e+01 1.1e+01 6.00 -87269 316.4560 +47.1921 1400 [WBH2005] G88.468-0.001 1.44e+02 2.9e+01 6.00 -87269 316.4594 +47.2030 1410 RRF 802 2.90e+02 5.8e+01 564.00 87269 316.4437 +47.1806 2700 F3R 2853 1.40e+02 2.8e+01 150.00 87269 316.4504 +47.1953 4850 87GB 210403.6+465922 6.38e+01 1.3e+01 138.00 87269 316.4488 +47.1903

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