Complement to VIII/85A

Source VLSS_J1721.1+3543: 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  


   74  VLSS J1721.1+3541                 1.60e+03  3.2e+02      79.98   77480 6   -0.23    3.65  260.2925  +35.6914
   74  VLSS J1721.1+3543                 1.82e+03  3.6e+02      79.98   77480 6   -0.23    3.67  260.2842  +35.7189
  151  7C 171922.69+354515.00            1.98e+03  4.0e+02      70.20   77480 6   -0.21    3.62  260.2879  +35.7061
  325  WN B1719.3+3545                   1.56e+03  3.1e+02      12.00   77480 6   -0.23    3.67  260.2890  +35.7052
 1400  NVSS J172109+354216               8.19e+02  1.6e+02      45.00   77480 6   -0.21    3.62  260.2897  +35.7046
 1400  WB 1719+3545                      8.41e+02  1.7e+02     120.00   77480 6   -0.21    3.62  260.2929  +35.7044
 4885  RGB 1721+357                      7.84e+02  1.6e+02       4.02   77480 6   -0.23    3.67  260.2895  +35.7044
 8400  CLASS J172109.4908+354216.070     6.01e+02  1.2e+02       0.33   77480 6   -0.23    3.67  260.2895  +35.7045
 8400  JVAS J1721+357                    5.84e+02  1.2e+02       0.33   77480 6   -0.23    3.67  260.2895  +35.7045
10700  RGB2 J1721.2+3542                 3.57e+02  7.1e+01      72.00   77480 6   -0.41    4.19  260.2912  +35.7069

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 J1721.1+3541                 1.60e+03  3.2e+02      79.98    77480  260.2925  +35.6914
    74  VLSS J1721.1+3543                 1.82e+03  3.6e+02      79.98    77480  260.2842  +35.7189
   151  7C 171922.69+354515.00            1.98e+03  4.0e+02      70.20    77480  260.2879  +35.7061
   232  MY 171923.9+354231.2              1.29e+03  2.6e+02     150.00   -77480  260.2929  +35.7087
   325  WN B1719.3+3545                   1.56e+03  3.1e+02      12.00    77480  260.2890  +35.7052
   325  WN B1719.3+3545A                  7.78e+02  1.6e+02      12.00   -77480  260.2863  +35.7169
   325  WN B1719.3+3545B                  7.80e+02  1.6e+02      12.00   -77480  260.2916  +35.6932
   365  TXS 1719+357                      5.81e+02  1.2e+02       6.00   -77480  260.2858  +35.7153
   408  B2.3 1719+35                      1.15e+03  2.3e+02       0.00   -77480  260.2887  +35.7133
  1400  FIRST J172107.7+354317            2.30e+01  4.6e+00       5.00   -77480  260.2824  +35.7216
  1400  FIRST J172108.3+354306            2.14e+01  4.3e+00       5.00   -77480  260.2848  +35.7184
  1400  FIRST J172108.9+354313            3.82e+01  7.6e+00       5.00   -77480  260.2873  +35.7205
  1400  FIRST J172109.5+354215            3.93e+02  7.9e+01       5.00   -77480  260.2897  +35.7044
  1400  FIRST J172109.6+354139            3.54e+01  7.1e+00       5.00   -77480  260.2902  +35.6942
  1400  FIRST J172109.7+354116            1.63e+01  3.3e+00       5.00   -77480  260.2906  +35.6880
  1400  FIRST J172110.2+354108            1.42e+01  2.8e+00       5.00   -77480  260.2927  +35.6856
  1400  FIRST J172110.3+354118            2.77e+01  5.5e+00       5.00   -77480  260.2930  +35.6885
  1400  NVSS J172109+354216               8.19e+02  1.6e+02      45.00    77480  260.2897  +35.7046
  1400  WB 1719+3545                      8.41e+02  1.7e+02     120.00    77480  260.2929  +35.7044
  2700  RGB11 J1721.2+3542                6.76e+02  1.4e+02     258.00   -77480  260.2912  +35.7069
  4850  GB6 B1719+3545                    7.84e+02  1.6e+02     108.00   -77480  260.2917  +35.7047
  4850  MITG J172109+3542                 6.45e+02  1.3e+02     258.00   -77480  260.2896  +35.7111
  4885  RGB 1721+357                      7.84e+02  1.6e+02       4.02    77480  260.2895  +35.7044
  5000  RGB6 J1721.2+3542                 5.26e+02  1.1e+02     144.00   -77480  260.2912  +35.7069
  8400  CLASS J172109.4908+354216.070     6.01e+02  1.2e+02       0.33    77480  260.2895  +35.7045
 10700  RGB2 J1721.2+3542                 3.57e+02  7.1e+01      72.00    77480  260.2912  +35.7069

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