Complement to VIII/85A

Source NVSS_J073855+384630: 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 073532.60+385315.00 5.57e+02 1.1e+02 70.20 31566 6 -0.75 4.47 114.7304 +38.7728 232 MY 073530.5+384629.7 2.40e+02 6.7e+01 150.00 31566 6 -0.65 4.05 114.7221 +38.7749 232 MY 073534.5+384546.5 2.80e+02 5.6e+01 150.00 31566 6 -0.65 4.05 114.7383 +38.7629 325 WN B0735.5+3853 3.70e+02 7.4e+01 12.00 31566 6 -0.71 4.36 114.7318 +38.7730 408 B2.3 0735+38 4.15e+02 8.3e+01 0.00 31566 6 -0.78 4.52 114.7221 +38.7850 408 B3 0735+388 3.60e+02 7.2e+01 84.00 31566 6 -0.75 4.47 114.7354 +38.7689 1400 NVSS J073855+384630 1.30e+02 2.6e+01 45.00 31566 6 -0.75 4.46 114.7307 +38.7752 4850 87GB 073529.0+385210 6.53e+01 1.3e+01 138.00 31566 6 -0.71 4.36 114.7154 +38.7550 4850 BWE 0735+3853 3.60e+01 7.2e+00 138.00 31566 6 -0.65 4.05 114.7317 +38.7706 4850 GB6 B0735+3852 6.34e+01 1.3e+01 108.00 31566 6 -0.76 4.50 114.7258 +38.7647 10600 B3VLA 327 2.80e+01 5.6e+00 69.00 31566 6 -0.75 4.47 114.7308 +38.7722

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 J0738.9+3846 6.10e+02 1.2e+02 79.98 -31566 114.7325 +38.7697 151 7C 073532.60+385315.00 5.57e+02 1.1e+02 70.20 31566 114.7304 +38.7728 232 MY 073530.5+384629.7 2.40e+02 6.7e+01 150.00 31566 114.7221 +38.7749 232 MY 073534.5+384546.5 2.80e+02 5.6e+01 150.00 31566 114.7383 +38.7629 325 WN B0735.5+3853 3.70e+02 7.4e+01 12.00 31566 114.7318 +38.7730 408 B2.3 0735+38 4.15e+02 8.3e+01 0.00 31566 114.7221 +38.7850 408 B3 0735+388 3.60e+02 7.2e+01 84.00 31566 114.7354 +38.7689 1400 FIRST J073854.4+384647 2.29e+01 4.6e+00 5.00 -31566 114.7268 +38.7798 1400 FIRST J073854.7+384628 2.63e+01 5.3e+00 5.00 -31566 114.7283 +38.7746 1400 FIRST J073855.3+384649 3.27e+01 6.5e+00 5.00 -31566 114.7306 +38.7803 1400 FIRST J073856.7+384552 3.70e+01 7.4e+00 5.00 -31566 114.7366 +38.7647 1400 NVSS J073855+384630 1.30e+02 2.6e+01 45.00 31566 114.7307 +38.7752 4730 B3a 0735+388 4.60e+01 9.2e+00 168.00 -31566 114.7356 +38.7691 4850 87GB 073529.0+385210 6.53e+01 1.3e+01 138.00 31566 114.7154 +38.7550 4850 BWE 0735+3853 3.60e+01 7.2e+00 138.00 31566 114.7317 +38.7706 4850 GB6 B0735+3852 6.34e+01 1.3e+01 108.00 31566 114.7258 +38.7647 10600 B3VLA 327 2.80e+01 5.6e+00 69.00 31566 114.7308 +38.7722

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