Complement to VIII/85A

Source RFS_1154: 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 B2014.6+3509 5.84e+02 1.2e+02 12.00 83773 0 -0.79 4.75 304.1280 +35.3118 327 WSRTGP 2014+3509 4.52e+02 9.0e+01 60.00 83773 0 -0.79 4.74 304.1280 +35.3131 365 TXS 2014+351 5.15e+02 1.0e+02 6.00 83773 0 -0.79 4.75 304.1278 +35.3134 408 B2.3 2014+35B 5.43e+02 1.1e+02 0.00 83773 0 -0.77 4.69 304.1275 +35.3133 408 DRAOP 14P36 6.97e+02 1.4e+02 210.00 83773 0 -0.77 4.69 304.1220 +35.3203 1400 NVSS J201630+351847 1.81e+02 3.6e+01 45.00 83773 0 -0.79 4.75 304.1277 +35.3132 1410 RRF 673 1.90e+02 3.8e+01 564.00 83773 0 -0.77 4.69 304.1308 +35.3019 2695 RFS 1154 1.10e+02 2.2e+01 294.00 83773 0 -0.77 4.69 304.1250 +35.3167 2700 F3R 2486 1.10e+02 2.2e+01 150.00 83773 0 -0.77 4.69 304.1254 +35.3167 4850 87GB 201435.4+350921 7.30e+01 1.5e+01 138.00 83773 0 -0.77 4.69 304.1250 +35.3111 4850 BWE 2014+3509 6.90e+01 1.4e+01 138.00 83773 0 -0.77 4.69 304.1263 +35.3103 4850 GB6 B2014+3509 7.30e+01 1.5e+01 108.00 83773 0 -0.77 4.69 304.1250 +35.3119 4850 MITG J201627+3518 4.90e+01 9.8e+00 258.00 83773 0 -0.77 4.69 304.1162 +35.3000 4850 MITG J201629+3519 6.80e+01 1.4e+01 258.00 83773 0 -0.77 4.69 304.1221 +35.3203

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 B2014.6+3509 5.84e+02 1.2e+02 12.00 83773 304.1280 +35.3118 327 WSRTGP 2014+3509 4.52e+02 9.0e+01 60.00 83773 304.1280 +35.3131 365 TXS 2014+351 5.15e+02 1.0e+02 6.00 83773 304.1278 +35.3134 408 B2.3 2014+35B 5.43e+02 1.1e+02 0.00 83773 304.1275 +35.3133 408 DRAOP 14P36 6.97e+02 1.4e+02 210.00 83773 304.1220 +35.3203 1400 GPSR 073.429+0.011 5.70e+01 1.1e+01 5.00 -83773 304.1246 +35.3137 1400 GPSR 073.430+0.007 7.20e+01 1.4e+01 5.00 -83773 304.1292 +35.3126 1400 NVSS J201630+351847 1.81e+02 3.6e+01 45.00 83773 304.1277 +35.3132 1400 [WBH2005] G73.429+0.011 4.74e+01 9.5e+00 6.00 -83773 304.1247 +35.3137 1400 [WBH2005] G73.430+0.007 7.87e+01 1.6e+01 6.00 -83773 304.1294 +35.3125 1410 RRF 673 1.90e+02 3.8e+01 564.00 83773 304.1308 +35.3019 2695 RFS 1154 1.10e+02 2.2e+01 294.00 83773 304.1250 +35.3167 2700 F3R 2486 1.10e+02 2.2e+01 150.00 83773 304.1254 +35.3167 4850 GB6 B2014+3509 7.30e+01 1.5e+01 108.00 83773 304.1250 +35.3119 4850 MITG J201627+3518 4.90e+01 9.8e+00 258.00 83773 304.1162 +35.3000

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