Complement to VIII/85A

Source GB6_B0754+3937: 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
325 WN B0754.7+3937 1.99e+03 4.0e+02 12.00 32221 0 -1.24 6.70 119.5368 +39.4909 365 TXS 0754+396 1.89e+03 3.8e+02 6.00 32221 0 -1.24 6.70 119.5370 +39.4910 408 B2.3 0754+39 1.26e+03 2.5e+02 0.00 32221 0 -1.00 5.70 119.5354 +39.4767 408 B3 0754+396 1.53e+03 3.1e+02 84.00 32221 0 -1.00 5.70 119.5383 +39.4903 1400 FIRST J075808.8+392928 5.22e+02 1.0e+02 5.00 32221 0 -1.24 6.70 119.5368 +39.4911 1400 NVSS J075808+392928 5.45e+02 1.1e+02 45.00 32221 0 -1.24 6.70 119.5368 +39.4913 1400 WB 0754+3937 5.55e+02 1.1e+02 120.00 32221 0 -1.24 6.70 119.5346 +39.4886 4730 B3a 0754+396 1.48e+02 3.0e+01 168.00 32221 0 -1.00 5.70 119.5382 +39.4906 4850 87GB 075446.4+393725 1.34e+02 2.7e+01 138.00 32221 0 -1.00 5.71 119.5346 +39.4883 4850 BWE 0754+3937 1.32e+02 2.6e+01 138.00 32221 0 -1.00 5.70 119.5346 +39.4886 4850 GB6 B0754+3937 1.37e+02 2.7e+01 108.00 32221 0 -1.00 5.70 119.5304 +39.4889 4860 [FPD2001b]a 77 1.05e+02 2.1e+01 0.40 32221 0 -1.00 5.70 119.5369 +39.4910 8460 [FPD2001b]b 77 5.57e+01 1.1e+01 0.20 32221 0 -1.00 5.70 119.5369 +39.4910 10600 B3VLA 364 4.89e+01 9.8e+00 69.00 32221 0 -1.24 6.70 119.5367 +39.4908

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 J0758.1+3929 5.61e+03 1.1e+03 79.98 -32221 119.5371 +39.4911 151 7C 075446.79+393735.00 3.19e+03 6.4e+02 70.20 -32221 119.5362 +39.4908 178 4C +39.21 2.90e+03 8.7e+02 690.00 -32221 119.5279 +39.5350 232 MY 075446.4+392929.3 2.17e+03 4.3e+02 150.00 -32221 119.5350 +39.4915 325 WN B0754.7+3937 1.99e+03 4.0e+02 12.00 32221 119.5368 +39.4909 365 TXS 0754+396 1.89e+03 3.8e+02 6.00 32221 119.5370 +39.4910 408 B2.3 0754+39 1.26e+03 2.5e+02 0.00 32221 119.5354 +39.4767 408 B3 0754+396 1.53e+03 3.1e+02 84.00 32221 119.5383 +39.4903 1400 FIRST J075808.3+392919 5.70e+00 1.1e+00 5.00 -32221 119.5346 +39.4886 1400 WB 0754+3937 5.55e+02 1.1e+02 120.00 32221 119.5346 +39.4886 4730 B3a 0754+396 1.48e+02 3.0e+01 168.00 32221 119.5382 +39.4906 4850 GB6 B0754+3937 1.37e+02 2.7e+01 108.00 32221 119.5304 +39.4889 4860 [FPD2001b]a 76 3.80e+01 7.6e+00 0.40 -32221 119.5330 +39.4812 8460 [FPD2001b]b 77 5.57e+01 1.1e+01 0.20 32221 119.5369 +39.4910 10600 B3VLA 364 4.89e+01 9.8e+00 69.00 32221 119.5367 +39.4908

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