Complement to VIII/85A

Source MITG_J183559+2506: 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
1400 NVSS J183558+250644 3.22e+01 6.4e+00 45.00 80508 0 1.15 -2.24 278.9931 +25.1124 4850 87GB 183356.2+250411 1.41e+02 2.8e+01 138.00 80508 0 0.93 -1.42 278.9962 +25.1119 4850 BWE 1833+2504 1.38e+02 2.8e+01 138.00 80508 0 0.96 -1.52 278.9971 +25.1119 4850 GB6 B1833+2504 1.31e+02 2.6e+01 108.00 80508 0 0.96 -1.52 278.9950 +25.1117 4850 MITG J183558+2507 1.18e+02 2.4e+01 258.00 80508 0 0.96 -1.52 278.9950 +25.1175 4850 MITG J183559+2506 1.00e+02 2.0e+01 258.00 80508 0 0.93 -1.42 278.9991 +25.1033 8400 CLASS J183558.3808+250645.402 1.81e+02 3.6e+01 0.33 80508 0 0.93 -1.42 278.9933 +25.1126 8400 JVAS J1835+2506 1.71e+02 3.4e+01 0.33 80508 0 0.93 -1.42 278.9932 +25.1126
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
No object found

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