Complement to VIII/85A

Source WN_B2356.9+3833: 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
325 WN B2356.9+3833 3.75e+02 7.5e+01 12.00 107335 4 0.23 1.87 359.8881 +38.8448 365 TXS 2356+385 2.58e+02 5.2e+01 6.00 107335 4 0.23 1.87 359.8878 +38.8456 408 B2.3 2357+38 3.06e+02 6.1e+01 0.00 107335 4 0.23 1.89 359.8929 +38.8550 408 B3 2356+385 3.00e+02 6.0e+01 84.00 107335 4 0.18 2.01 359.8875 +38.8483 1400 NVSS J235933+385042 5.24e+02 1.0e+02 45.00 107335 4 0.23 1.87 359.8882 +38.8452 1400 WB 2356+3833 6.42e+02 1.3e+02 120.00 107335 4 0.18 2.01 359.8863 +38.8444 4850 87GB 235659.1+383358 4.49e+02 9.0e+01 138.00 107335 4 0.15 2.08 359.8854 +38.8444 4850 GB6 B2356+3833 4.79e+02 9.6e+01 108.00 107335 4 0.18 2.01 359.8879 +38.8444 4850 MITG J235930+3849 5.00e+02 1.0e+02 258.00 107335 4 0.21 1.94 359.8788 +38.8206 4850 MITG J235932+3850 5.36e+02 1.1e+02 258.00 107335 4 0.13 2.24 359.8867 +38.8406

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
325 WN B2356.9+3833 3.75e+02 7.5e+01 12.00 107335 359.8881 +38.8448 365 TXS 2356+385 2.58e+02 5.2e+01 6.00 107335 359.8878 +38.8456 408 B2.3 2357+38 3.06e+02 6.1e+01 0.00 107335 359.8929 +38.8550 408 B3 2356+385 3.00e+02 6.0e+01 84.00 107335 359.8875 +38.8483 1400 NVSS J235933+385042 5.24e+02 1.0e+02 45.00 107335 359.8882 +38.8452 1400 WB 2356+3833 6.42e+02 1.3e+02 120.00 107335 359.8863 +38.8444 4850 87GB 235659.1+383358 4.49e+02 9.0e+01 138.00 107335 359.8854 +38.8444 4850 BWE 2356+3833 4.37e+02 8.7e+01 138.00 -107335 359.8863 +38.8444 4850 GB6 B2356+3833 4.79e+02 9.6e+01 108.00 107335 359.8879 +38.8444 4850 MITG J235930+3849 5.00e+02 1.0e+02 258.00 107335 359.8788 +38.8206 4850 MITG J235932+3850 5.36e+02 1.1e+02 258.00 107335 359.8867 +38.8406 8400 CLASS J235932.6233+385033.243 1.29e+01 2.6e+00 0.33 -107335 359.8859 +38.8426 8400 CLASS J235932.8019+385042.636 1.84e+01 3.7e+00 0.33 -107335 359.8867 +38.8452 8400 CLASS J235932.9050+385037.884 1.14e+01 2.3e+00 0.33 -107335 359.8871 +38.8439 8400 CLASS J235933.1796+385042.334 2.48e+02 5.0e+01 0.33 -107335 359.8882 +38.8451 8400 CLASS J235933.5572+385042.058 1.74e+01 3.5e+00 0.33 -107335 359.8898 +38.8450 8400 CLASS J235933.6670+385030.935 8.10e+00 1.6e+00 0.33 -107335 359.8902 +38.8419 8400 JVAS J2359+388 2.78e+02 5.6e+01 0.33 -107335 359.8883 +38.8451

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