Complement to VIII/85A

Source WN_B1827.1+3218: 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
232 MY 182701.0+321931.2 5.90e+02 1.2e+02 150.00 80288 7 -0.61 4.07 277.2200 +32.3253 325 WN B1827.0+3218 7.26e+02 1.5e+02 12.00 80288 7 -0.55 4.15 277.2364 +32.3370 325 WN B1827.0+3218A 3.03e+02 6.1e+01 12.00 80288 7 -0.61 4.07 277.2206 +32.3132 325 WN B1827.1+3218 7.51e+02 1.5e+02 12.00 80288 7 -0.55 4.15 277.2421 +32.3380 325 WN B1827.1+3218A 4.67e+02 9.3e+01 12.00 80288 7 -0.71 4.45 277.2261 +32.3191 1400 NVSS J182852+321855 1.62e+02 3.2e+01 45.00 80288 7 -0.71 4.45 277.2204 +32.3153 1400 WB 1827+3217 3.25e+02 6.5e+01 120.00 80288 7 -0.53 4.11 277.2379 +32.3311 4850 87GB 182705.4+321752 1.39e+02 2.8e+01 138.00 80288 7 -0.48 3.90 277.2387 +32.3317 4850 BWE 1827+3217 1.34e+02 2.7e+01 138.00 80288 7 -0.55 4.15 277.2379 +32.3311 4850 GB6 B1827+3217 1.32e+02 2.6e+01 108.00 80288 7 -0.49 3.93 277.2417 +32.3292 4850 MITG J182852+3219 6.90e+01 1.4e+01 258.00 80288 7 -0.71 4.45 277.2200 +32.3272 4850 MITG J182858+3219 7.00e+01 1.4e+01 258.00 80288 7 -0.70 4.43 277.2433 +32.3306

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 J1828.8+3218 8.70e+02 1.7e+02 79.98 -80288 277.2200 +32.3161 232 MY 182701.0+321931.2 5.90e+02 1.2e+02 150.00 80288 277.2200 +32.3253 325 WN B1827.0+3218 7.26e+02 1.5e+02 12.00 80288 277.2364 +32.3370 325 WN B1827.0+3218A 3.03e+02 6.1e+01 12.00 80288 277.2206 +32.3132 325 WN B1827.0+3218B 1.94e+02 3.9e+01 12.00 -80288 277.2353 +32.3302 325 WN B1827.1+3218 7.51e+02 1.5e+02 12.00 80288 277.2421 +32.3380 325 WN B1827.1+3218A 4.67e+02 9.3e+01 12.00 80288 277.2261 +32.3191 408 B2.1 1827+32A 5.20e+02 1.0e+02 0.00 -80288 277.2271 +32.3233 1400 NVSS J182852+321855 1.62e+02 3.2e+01 45.00 80288 277.2204 +32.3153 1400 NVSS J182856+322002 6.93e+01 1.4e+01 45.00 -80288 277.2373 +32.3339 1400 NVSS J182902+322040 6.40e+00 1.3e+00 45.00 -80288 277.2591 +32.3447 1400 WB 1827+3217 3.25e+02 6.5e+01 120.00 80288 277.2379 +32.3311 4850 87GB 182705.4+321752 1.39e+02 2.8e+01 138.00 80288 277.2387 +32.3317 4850 MITG J182852+3219 6.90e+01 1.4e+01 258.00 80288 277.2200 +32.3272 4850 MITG J182858+3219 7.00e+01 1.4e+01 258.00 80288 277.2433 +32.3306 8400 CLASS J182856.9316+322004.128 1.67e+01 3.3e+00 0.33 -80288 277.2372 +32.3345

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