Complement to VIII/85A

Source WB_1018+4538: 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
74 VLSS J1021.1+4523 1.01e+03 2.0e+02 79.98 41546 0 -0.66 4.23 155.2779 +45.3939 151 6C 101804+453853 6.50e+02 1.3e+02 252.00 41546 0 -0.66 4.23 155.2775 +45.3961 151 7C 101803.39+453837.00 6.62e+02 1.3e+02 70.20 41546 0 -0.66 4.23 155.2750 +45.3914 325 WN B1018.0+4538 3.51e+02 7.0e+01 12.00 41546 0 -0.66 4.23 155.2752 +45.3914 408 51P 134 3.29e+02 6.6e+01 240.00 41546 0 -0.66 4.23 155.2741 +45.3890 408 B3 1018+456 2.60e+02 5.2e+01 84.00 41546 0 -0.54 3.89 155.2754 +45.3922 1400 NVSS J102106+452328 1.27e+02 2.5e+01 45.00 41546 0 -0.68 4.28 155.2751 +45.3912 1400 WB 1018+4538 1.77e+02 3.5e+01 120.00 41546 0 -0.56 3.98 155.2717 +45.3925 4850 87GB 101802.1+453842 8.90e+01 1.8e+01 138.00 41546 0 -0.66 4.23 155.2696 +45.3931 4850 GB6 B1018+4538 8.20e+01 1.6e+01 108.00 41546 0 -0.66 4.23 155.2738 +45.3922 4885 RGB 1021+453 8.20e+01 1.6e+01 4.02 41546 0 -0.66 4.23 155.2751 +45.3922 8400 CLASS J102106.0438+452331.797 4.00e+01 8.0e+00 0.33 41546 0 -0.66 4.23 155.2752 +45.3922

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 J1021.1+4523 1.01e+03 2.0e+02 79.98 41546 155.2779 +45.3939 151 6C 101804+453853 6.50e+02 1.3e+02 252.00 41546 155.2775 +45.3961 151 7C 101803.39+453837.00 6.62e+02 1.3e+02 70.20 41546 155.2750 +45.3914 232 MY 101758.0+452330.9 2.10e+02 6.4e+01 150.00 -41546 155.2525 +45.3919 325 WN B1018.0+4538 3.51e+02 7.0e+01 12.00 41546 155.2752 +45.3914 365 TXS 1017+456 2.90e+02 5.8e+01 6.00 -41546 155.2542 +45.4072 408 51P 134 3.29e+02 6.6e+01 240.00 41546 155.2741 +45.3890 408 B3 1018+456 2.60e+02 5.2e+01 84.00 41546 155.2754 +45.3922 1400 FIRST J102105.8+452347 1.93e+01 3.9e+00 5.00 -41546 155.2746 +45.3966 1400 FIRST J102105.9+452323 4.14e+01 8.3e+00 5.00 -41546 155.2749 +45.3898 1400 FIRST J102106.0+452331 4.29e+01 8.6e+00 5.00 -41546 155.2751 +45.3921 1400 FIRST J102106.3+452316 1.66e+01 3.3e+00 5.00 -41546 155.2763 +45.3880 1400 WB 1018+4538 1.77e+02 3.5e+01 120.00 41546 155.2717 +45.3925 4850 87GB 101802.1+453842 8.90e+01 1.8e+01 138.00 41546 155.2696 +45.3931 4885 RGB 1021+453 8.20e+01 1.6e+01 4.02 41546 155.2751 +45.3922 8400 CLASS J102106.0438+452331.797 4.00e+01 8.0e+00 0.33 41546 155.2752 +45.3922

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