Complement to VIII/85A

Source F3R_4653: 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
151 7C 044601.80+421240.00 2.51e+03 5.0e+02 70.20 17800 5 -0.55 4.67 072.3883 +42.2975 178 4C +42.14 2.30e+03 6.9e+02 690.00 17800 5 -0.53 4.62 072.3942 +42.2700 232 MY 044601.0+421751.3 2.32e+03 4.6e+02 150.00 17800 5 -0.55 4.67 072.3850 +42.2976 325 WN B0446.0+4212 2.74e+03 5.5e+02 12.00 17800 5 -0.55 4.67 072.3893 +42.2964 365 TXS 0446+422 2.28e+03 4.6e+02 6.00 17800 5 -0.55 4.67 072.3902 +42.2963 408 32P 126 2.40e+03 4.8e+02 240.00 17800 5 -0.53 4.62 072.3872 +42.2990 408 B3 0446+422 2.12e+03 4.2e+02 84.00 17800 5 -0.55 4.67 072.3883 +42.2947 1400 NVSS J044933+421747 8.96e+02 1.8e+02 45.00 17800 5 -0.55 4.67 072.3899 +42.2966 1400 WB 0446+4212 1.25e+03 2.5e+02 120.00 17800 5 -0.74 5.24 072.3817 +42.2947 1410 RRF 1730 8.56e+02 1.7e+02 564.00 17800 5 -0.53 4.62 072.3912 +42.2967 2700 F3R 4653 5.60e+02 1.1e+02 150.00 17800 5 -0.55 4.67 072.3983 +42.2919 4850 87GB 044600.1+421233 3.82e+02 7.6e+01 138.00 17800 5 -0.53 4.62 072.3812 +42.2956 4850 BWE 0446+4212 3.42e+02 6.8e+01 138.00 17800 5 -0.55 4.67 072.3817 +42.2947 4850 GB6 B0446+4212 3.28e+02 6.6e+01 108.00 17800 5 -0.74 5.24 072.3846 +42.2956

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 J0449.5+4217 1.39e+03 2.8e+02 79.98 -17800 072.3867 +42.2983 151 7C 044601.80+421240.00 2.51e+03 5.0e+02 70.20 17800 072.3883 +42.2975 178 4C +42.14 2.30e+03 6.9e+02 690.00 17800 072.3942 +42.2700 232 MY 044601.0+421751.3 2.32e+03 4.6e+02 150.00 17800 072.3850 +42.2976 325 WN B0446.0+4212 2.74e+03 5.5e+02 12.00 17800 072.3893 +42.2964 325 WN B0446.5+4209 4.30e+01 8.6e+00 12.00 -17800 072.5095 +42.2499 365 TXS 0446+422 2.28e+03 4.6e+02 6.00 17800 072.3902 +42.2963 408 32P 126 2.40e+03 4.8e+02 240.00 17800 072.3872 +42.2990 1400 NVSS J044929+421835 4.84e+01 9.7e+00 45.00 -17800 072.3725 +42.3098 1400 NVSS J045001+421445 1.13e+01 2.3e+00 45.00 -17800 072.5055 +42.2460 1400 WB 0446+4212 1.25e+03 2.5e+02 120.00 17800 072.3817 +42.2947 1410 RRF 1730 8.56e+02 1.7e+02 564.00 17800 072.3912 +42.2967 2700 F3R 4653 5.60e+02 1.1e+02 150.00 17800 072.3983 +42.2919 4850 87GB 044600.1+421233 3.82e+02 7.6e+01 138.00 17800 072.3812 +42.2956 4850 BWE 0446+4212 3.42e+02 6.8e+01 138.00 17800 072.3817 +42.2947

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