Complement to VIII/85A

Source B3a_0722+393: 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
178 4C +39.17 2.80e+03 8.4e+02 690.00 31093 4 -1.01 6.11 111.4562 +39.3283 325 WN B0722.4+3923 3.57e+03 7.1e+02 12.00 31093 4 -1.01 6.11 111.4586 +39.2901 365 TXS 0722+393 3.27e+03 6.5e+02 6.00 31093 4 -1.01 6.11 111.4583 +39.2904 408 B2.3 0722+39 2.84e+03 5.7e+02 0.00 31093 4 -1.01 6.11 111.4592 +39.2933 408 B3 0722+393A 2.91e+03 5.8e+02 84.00 31093 4 -1.01 6.11 111.4583 +39.2911 1400 FIRST J072549.9+391725 1.07e+03 2.1e+02 5.00 31093 4 -1.01 6.11 111.4583 +39.2904 1400 NVSS J072550+391725 1.10e+03 2.2e+02 45.00 31093 4 -1.01 6.11 111.4585 +39.2905 1400 WB 0722+3923 1.12e+03 2.2e+02 120.00 31093 4 -1.00 6.08 111.4558 +39.2889 4730 B3a 0722+393 2.42e+02 4.8e+01 168.00 31093 4 -0.82 5.30 111.4581 +39.2913 4850 87GB 072224.5+392321 2.36e+02 4.7e+01 138.00 31093 4 -0.82 5.30 111.4554 +39.2892 4850 BWE 0722+3923 2.32e+02 4.6e+01 138.00 31093 4 -1.01 6.09 111.4558 +39.2889 4850 GB6 B0722+3923 2.43e+02 4.9e+01 108.00 31093 4 -0.82 5.30 111.4546 +39.2900 8460 [FPD2001b]b 68 1.17e+02 2.3e+01 0.20 31093 4 -1.01 6.11 111.4583 +39.2904

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 J0725.8+3917 3.02e+03 6.0e+02 79.98 -31093 111.4583 +39.2914 151 7C 072225.10+392324.00 2.86e+03 5.7e+02 70.20 -31093 111.4579 +39.2900 178 4C +39.17 2.80e+03 8.4e+02 690.00 31093 111.4562 +39.3283 232 MY 072225.4+391726.8 3.16e+03 6.3e+02 150.00 -31093 111.4596 +39.2908 325 WN B0722.4+3923 3.57e+03 7.1e+02 12.00 31093 111.4586 +39.2901 365 TXS 0722+393 3.27e+03 6.5e+02 6.00 31093 111.4583 +39.2904 408 B2.3 0722+39 2.84e+03 5.7e+02 0.00 31093 111.4592 +39.2933 408 B3 0722+393A 2.91e+03 5.8e+02 84.00 31093 111.4583 +39.2911 1400 FIRST J072544.7+391808 1.80e+00 4.0e-01 5.00 -31093 111.4365 +39.3024 1400 FIRST J072551.3+391716 7.00e-01 2.0e-01 5.00 -31093 111.4639 +39.2880 1400 WB 0722+3923 1.12e+03 2.2e+02 120.00 31093 111.4558 +39.2889 4730 B3a 0722+393 2.42e+02 4.8e+01 168.00 31093 111.4581 +39.2913 4850 GB6 B0722+3923 2.43e+02 4.9e+01 108.00 31093 111.4546 +39.2900 8460 [FPD2001b]b 68 1.17e+02 2.3e+01 0.20 31093 111.4583 +39.2904 8460 [FPD2001b]b 69 8.90e+00 1.8e+00 0.20 -31093 111.4583 +39.2903 10600 B3VLA 312 5.98e+01 1.2e+01 69.00 -31093 111.4579 +39.2922

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