Complement to VIII/85A

Source 7C_091253.50+294557.00: 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 J0915.8+2933 9.30e+02 1.9e+02 79.98 39323 0 -0.35 3.64 138.9692 +29.5556 151 7C 091253.50+294557.00 7.81e+02 1.6e+02 70.20 39323 0 -0.35 3.64 138.9683 +29.5569 325 WN B0912.8+2945 5.95e+02 1.2e+02 12.00 39323 0 -0.35 3.64 138.9684 +29.5569 365 TXS 0912+297 5.56e+02 1.1e+02 6.00 39323 0 -0.35 3.64 138.9679 +29.5566 408 B2.1 0912+29 5.10e+02 1.0e+02 0.00 39323 0 -0.35 3.64 138.9671 +29.5617 1400 FIRST J091552.3+293324 3.56e+02 7.1e+01 5.00 39323 0 -0.35 3.64 138.9683 +29.5567 1400 NVSS J091552+293324 3.42e+02 6.8e+01 45.00 39323 0 -0.35 3.64 138.9683 +29.5567 1400 WB 0912+2946 3.27e+02 6.5e+01 120.00 39323 0 -0.35 3.64 138.9683 +29.5597 2700 RGB11 J0915.9+2933 3.38e+02 6.8e+01 258.00 39323 0 -0.35 3.64 138.9688 +29.5594 4850 87GB 091253.6+294605 2.28e+02 4.6e+01 138.00 39323 0 -0.35 3.64 138.9688 +29.5594 4850 BWE 0912+2946 2.25e+02 4.5e+01 138.00 39323 0 -0.35 3.64 138.9683 +29.5597 4850 GB6 B0912+2945 2.15e+02 4.3e+01 108.00 39323 0 -0.36 3.66 138.9725 +29.5572 4850 MITG J091550+2933 2.27e+02 4.5e+01 258.00 39323 0 -0.35 3.64 138.9621 +29.5581 4885 RGB 0915+295 2.15e+02 4.3e+01 4.02 39323 0 -0.35 3.64 138.9683 +29.5566 5000 RGB6 J0915.9+2933 2.72e+02 5.4e+01 144.00 39323 0 -0.35 3.64 138.9688 +29.5594 8400 CLASS J091552.4014+293323.981 1.86e+02 3.7e+01 0.33 39323 0 -0.35 3.64 138.9683 +29.5567 8400 JVAS J0915+2933 1.76e+02 3.5e+01 0.33 39323 0 -0.36 3.66 138.9683 +29.5567 15000 9C J0915+2933 1.48e+02 3.0e+01 25.20 39323 0 -0.35 3.64 138.9688 +29.5558

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 J0915.8+2933 9.30e+02 1.9e+02 79.98 39323 138.9692 +29.5556 151 7C 091253.50+294557.00 7.81e+02 1.6e+02 70.20 39323 138.9683 +29.5569 325 WN B0912.8+2945 5.95e+02 1.2e+02 12.00 39323 138.9684 +29.5569 408 B2.1 0912+29 5.10e+02 1.0e+02 0.00 39323 138.9671 +29.5617 1400 NVSS J091552+293324 3.42e+02 6.8e+01 45.00 39323 138.9683 +29.5567 4850 MITG J091550+2933 2.27e+02 4.5e+01 258.00 39323 138.9621 +29.5581 5000 RGB6 J0915.9+2933 2.72e+02 5.4e+01 144.00 39323 138.9688 +29.5594 8400 CLASS J091552.5833+293318.722 1.43e+01 2.9e+00 0.33 -39323 138.9691 +29.5552 15000 9C J0915+2933 1.48e+02 3.0e+01 25.20 39323 138.9688 +29.5558

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