Complement to VIII/85A

Source RRF_699: 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  


 1410  RRF 699                           1.32e+04  2.6e+03     564.00   86017 0   -0.10    4.41  305.4179  +37.4828
 4850  87GB 201945.9+372121              1.08e+04  2.2e+03     138.00   86017 0    0.02    4.04  305.4079  +37.5161
 4850  GB6 B2019+3721                    8.86e+03  1.8e+03     108.00   86017 0   -0.10    4.41  305.4104  +37.5172
 4850  MITG J202134+3731                 8.76e+03  1.8e+03     258.00   86017 0   -0.11    4.43  305.3946  +37.5192
 4850  MITG J202141+3731                 7.68e+03  1.5e+03     258.00   86017 0   -0.10    4.41  305.4208  +37.5261
 4850  MITG J202142+3731                 1.03e+04  2.1e+03     258.00   86017 0    0.02    4.04  305.4271  +37.5261
 8350  GPA1 075.83+0.38                  1.66e+04  3.3e+03     582.00   86017 0   -0.10    4.41  305.4292  +37.5011

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  


   325  WN B2019.7+3718                   3.93e+03  7.9e+02      12.00   -86017  305.4145  +37.4674
   325  WN B2019.7+3718B                  1.49e+03  3.0e+02      12.00   -86017  305.4093  +37.5203
   325  WN B2019.9+3720                   5.20e+01  1.0e+01      12.00   -86017  305.4564  +37.5018
   327  WSRTGP 2019+3720                  7.80e+01  1.6e+01      60.00   -86017  305.4577  +37.5011
   327  WSRTGP 2019+3721                  1.14e+03  2.3e+02      60.00   -86017  305.4093  +37.5203
   327  WSRTGP 2020+3723                  1.75e+02  3.5e+01      60.00   -86017  305.4966  +37.5456
   365  TXS 2019+373                      7.31e+02  1.5e+02       6.00   -86017  305.4092  +37.5192
   408  B2.3 2019+37                      4.41e+03  8.8e+02       0.00   -86017  305.4183  +37.4717
   408  DRAOP 14P50                       6.74e+03  1.3e+03     210.00   -86017  305.4179  +37.4681
  1400  GPSR 075.798+0.353                1.21e+02  2.4e+01       5.00   -86017  305.4337  +37.4628
  1400  GPSR 075.835+0.400                6.53e+03  1.3e+03       5.00   -86017  305.4119  +37.5197
  1400  NVSS J202138+373110               6.58e+03  1.3e+03      45.00   -86017  305.4111  +37.5195
  1400  NVSS J202149+373008               1.74e+02  3.5e+01      45.00   -86017  305.4553  +37.5023
  1400  NVSS J202157+373245               1.18e+01  2.4e+00      45.00   -86017  305.4892  +37.5460
  1400  [WBH2005] G75.832+0.403           1.73e+03  3.5e+02       6.00   -86017  305.4070  +37.5197
  1400  [WBH2005] G75.834+0.398           1.81e+03  3.6e+02       6.00   -86017  305.4134  +37.5181
  1400  [WBH2005] G75.836+0.401           1.15e+03  2.3e+02       6.00   -86017  305.4124  +37.5213
  1400  WSTB32W 46                        7.00e+03  1.4e+03      72.00   -86017  305.4108  +37.5186
  1410  RRF 699                           1.32e+04  2.6e+03     564.00    86017  305.4179  +37.4828
  2695  RFS 1184                          1.42e+04  2.8e+03     294.00   -86017  305.4229  +37.4956
  2700  F3R 2570                          1.42e+04  2.8e+03     150.00   -86017  305.4229  +37.4956
  2700  [PBD2003] G075.8+00.4             1.18e+04  2.5e+03     480.00   -86017  305.3858  +37.4897
  4850  87GB 201945.9+372121              1.08e+04  2.2e+03     138.00    86017  305.4079  +37.5161
  4850  MITG J202121+3730                 1.94e+03  3.9e+02     258.00   -86017  305.3383  +37.5097
  4850  MITG J202126+3725                 1.24e+03  2.5e+02     258.00   -86017  305.3600  +37.4303
  4850  MITG J202134+3731                 8.76e+03  1.8e+03     258.00    86017  305.3946  +37.5192
  4850  MITG J202141+3731                 7.68e+03  1.5e+03     258.00    86017  305.4208  +37.5261
  4850  MITG J202142+3731                 1.03e+04  2.1e+03     258.00    86017  305.4271  +37.5261
  4850  MITG J202154+3730                 9.22e+02  1.8e+02     258.00   -86017  305.4754  +37.5000
  8350  GPA1 075.83+0.38                  1.66e+04  3.3e+03     582.00    86017  305.4292  +37.5011

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