Complement to VIII/85A

Source 4C_+74.25: 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 J2017.2+7440 3.91e+03 7.8e+02 79.98 101168 0 -0.13 3.09 304.3079 +74.6794 151 6C 201759+743121 2.34e+03 4.7e+02 252.00 101168 0 -0.13 3.09 304.3042 +74.6797 178 4C +74.25 2.50e+03 7.5e+02 690.00 101168 0 -0.20 3.38 304.3183 +74.6950 232 MY 201800.5+744040.8 6.20e+02 1.2e+02 150.00 101168 0 -0.20 3.38 304.3092 +74.6780 325 WN B2017.9+7431 1.28e+03 2.6e+02 12.00 101168 0 -0.13 3.09 304.3042 +74.6801 1400 NVSS J201713+744047 4.73e+02 9.5e+01 45.00 101168 0 -0.20 3.38 304.3050 +74.6798 1400 WB 2017+7431 4.72e+02 9.4e+01 120.00 101168 0 -0.13 3.09 304.2979 +74.6794 2700 RGB11 J2017.2+7440 4.55e+02 9.1e+01 258.00 101168 0 -0.24 3.55 304.2979 +74.6794 4850 87GB 201757.4+743119 5.80e+02 1.2e+02 138.00 101168 0 -0.13 3.09 304.2962 +74.6792 4850 BWE 2017+7431 5.77e+02 1.2e+02 138.00 101168 0 -0.24 3.55 304.2979 +74.6794 4850 GB6 B2017+7431 5.35e+02 1.1e+02 108.00 101168 0 -0.13 3.09 304.3000 +74.6783 4885 RGB 2017+746 5.35e+02 1.1e+02 4.02 101168 0 -0.13 3.09 304.3045 +74.6800 5000 RGB6 J2017.2+7440 4.12e+02 8.2e+01 144.00 101168 0 -0.13 3.09 304.2979 +74.6794 8400 CLASS J201713.0787+744048.000 3.44e+02 6.9e+01 0.33 101168 0 -0.13 3.09 304.3044 +74.6800 8400 JVAS J2017+746 3.41e+02 6.8e+01 0.33 101168 0 -0.13 3.09 304.3045 +74.6800 10700 RGB2 J2017.2+7440 4.19e+02 8.4e+01 72.00 101168 0 -0.13 3.09 304.2979 +74.6794

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
38 8C 201758+743111 8.20e+03 1.6e+03 270.00 -101168 304.3000 +74.6769 74 VLSS J2017.2+7440 3.91e+03 7.8e+02 79.98 101168 304.3079 +74.6794 151 6C 201759+743121 2.34e+03 4.7e+02 252.00 101168 304.3042 +74.6797 178 4C +74.25 2.50e+03 7.5e+02 690.00 101168 304.3183 +74.6950 232 MY 201800.5+744040.8 6.20e+02 1.2e+02 150.00 101168 304.3092 +74.6780 325 WN B2017.9+7431 1.28e+03 2.6e+02 12.00 101168 304.3042 +74.6801 1400 NVSS J201713+744047 4.73e+02 9.5e+01 45.00 101168 304.3050 +74.6798 4850 87GB 201757.4+743119 5.80e+02 1.2e+02 138.00 101168 304.2962 +74.6792 4885 RGB 2017+746 5.35e+02 1.1e+02 4.02 101168 304.3045 +74.6800 5000 RGB6 J2017.2+7440 4.12e+02 8.2e+01 144.00 101168 304.2979 +74.6794 8400 CLASS J201713.0787+744048.000 3.44e+02 6.9e+01 0.33 101168 304.3044 +74.6800

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