Complement to VIII/85A

Source RGB_1707+135: 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]
2010A&A...511A..53V

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  


 2700  RGB11 J1707.8+1331                4.01e+02  8.0e+01     258.00   73561 0    0.51    0.73  256.9379  +13.5197
 4850  87GB 170527.4+133500              4.34e+02  8.7e+01     138.00   73561 0    0.51    0.73  256.9396  +13.5192
 4850  GB6 B1705+1335                    4.12e+02  8.2e+01     108.00   73561 0    0.51    0.73  256.9375  +13.5214
 4885  RGB 1707+135                      4.12e+02  8.2e+01       4.02   73561 0    0.51    0.73  256.9401  +13.5181
 8400  CLASS J170745.6349+133105.217     4.59e+02  9.2e+01       0.33   73561 0    0.51    0.73  256.9401  +13.5181
 8400  JVAS J1707+1331                   4.83e+02  9.7e+01       0.33   73561 0    0.51    0.73  256.9402  +13.5181

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]
2010A&A...511A..53V

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 J1707.7+1331                 7.00e+02  1.4e+02      79.98   -73561  256.9396  +13.5204
   365  TXS 1705+135                      4.14e+02  8.3e+01       6.00   -73561  256.9392  +13.5185
  1400  NVSS J170743+132928               1.04e+01  2.1e+00      45.00   -73561  256.9311  +13.4913
  1400  NVSS J170745+133105               3.02e+02  6.0e+01      45.00   -73561  256.9403  +13.5182
  1400  WB 1705+1335                      2.20e+02  4.4e+01     120.00   -73561  256.9396  +13.5194
  4850  87GB 170527.4+133500              4.34e+02  8.7e+01     138.00    73561  256.9396  +13.5192
  4850  BWE 1705+1335                     3.85e+02  7.7e+01     138.00   -73561  256.9396  +13.5194
  4850  MITG J170746+1331                 6.87e+02  1.4e+02     258.00   -73561  256.9429  +13.5175
  4885  RGB 1707+135                      4.12e+02  8.2e+01       4.02    73561  256.9401  +13.5181
  5000  RGB6 J1707.8+1331                 4.22e+02  8.4e+01     144.00   -73561  256.9379  +13.5197
  8400  CLASS J170745.6349+133105.217     4.59e+02  9.2e+01       0.33    73561  256.9401  +13.5181

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