Complement to VIII/85A

Source 87GB_134716.4+390645: 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  


  151  6C 134718+390652                  5.80e+02  1.2e+02     252.00   58586 4   -0.67    4.31  207.3629  +38.8667
  151  7C 134716.69+390633.00            7.40e+02  1.5e+02      70.20   58586 4   -0.64    4.20  207.3574  +38.8614
  232  MY 134718.3+385140.3              4.00e+02  9.3e+01     150.00   58586 4   -0.70    4.40  207.3642  +38.8612
  325  WN B1347.2+3906                   4.68e+02  9.4e+01      12.00   58586 4   -0.57    4.01  207.3578  +38.8616
  365  TXS 1347+391                      5.21e+02  1.0e+02       6.00   58586 4   -0.68    4.35  207.3577  +38.8618
  408  B2.3 1347+39C                     4.28e+02  8.6e+01       0.00   58586 4   -0.67    4.31  207.3542  +38.8700
  408  B3 1347+391                       4.40e+02  8.8e+01      84.00   58586 4   -0.70    4.40  207.3600  +38.8647
 1400  FIRST J134925.8+385142            1.62e+02  3.2e+01       5.00   58586 4   -0.68    4.35  207.3578  +38.8617
 1400  NVSS J134925+385143               1.79e+02  3.6e+01      45.00   58586 4   -0.73    4.55  207.3575  +38.8620
 1400  WB 1347+3906                      1.42e+02  2.8e+01     120.00   58586 4   -0.70    4.40  207.3575  +38.8633
 4730  B3a 1347+391                      7.10e+01  1.4e+01     168.00   58586 4   -0.64    4.20  207.3600  +38.8649
 4850  87GB 134716.4+390645              8.17e+01  1.6e+01     138.00   58586 4   -0.64    4.20  207.3567  +38.8647
 4850  BWE 1347+3906                     6.50e+01  1.3e+01     138.00   58586 4   -0.64    4.20  207.3575  +38.8633
 4850  GB6 B1347+3906                    6.99e+01  1.4e+01     108.00   58586 4   -0.64    4.20  207.3575  +38.8653

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 J1349.4+3851                 8.00e+02  1.6e+02      79.98   -58586  207.3571  +38.8622
   151  6C 134718+390652                  5.80e+02  1.2e+02     252.00    58586  207.3629  +38.8667
   151  7C 134716.69+390633.00            7.40e+02  1.5e+02      70.20    58586  207.3574  +38.8614
   232  MY 134718.3+385140.3              4.00e+02  9.3e+01     150.00    58586  207.3642  +38.8612
   325  WN B1347.2+3906                   4.68e+02  9.4e+01      12.00    58586  207.3578  +38.8616
   365  TXS 1347+391                      5.21e+02  1.0e+02       6.00    58586  207.3577  +38.8618
   408  B2.3 1347+39C                     4.28e+02  8.6e+01       0.00    58586  207.3542  +38.8700
   408  B3 1347+391                       4.40e+02  8.8e+01      84.00    58586  207.3600  +38.8647
  1400  FIRST J134923.2+385057            2.00e+00  4.0e-01       5.00   -58586  207.3468  +38.8494
  1400  FIRST J134924.8+385201            2.90e+00  6.0e-01       5.00   -58586  207.3535  +38.8671
  1400  FIRST J134925.5+385153            2.10e+00  4.0e-01       5.00   -58586  207.3566  +38.8649
  1400  FIRST J134925.8+385142            1.62e+02  3.2e+01       5.00    58586  207.3578  +38.8617
  1400  FIRST J134926.0+385131            2.00e+00  4.0e-01       5.00   -58586  207.3586  +38.8587
  1400  FIRST J134926.8+385122            2.40e+00  5.0e-01       5.00   -58586  207.3617  +38.8564
  1400  FIRST J134927.4+385136            9.00e-01  2.0e-01       5.00   -58586  207.3646  +38.8602
  1400  FIRST J134928.2+385225            2.20e+00  4.0e-01       5.00   -58586  207.3676  +38.8737
  1400  NVSS J134925+385143               1.79e+02  3.6e+01      45.00    58586  207.3575  +38.8620
  1400  WB 1347+3906                      1.42e+02  2.8e+01     120.00    58586  207.3575  +38.8633
  4730  B3a 1347+391                      7.10e+01  1.4e+01     168.00    58586  207.3600  +38.8649
  4850  87GB 134716.4+390645              8.17e+01  1.6e+01     138.00    58586  207.3567  +38.8647
  4850  BWE 1347+3906                     6.50e+01  1.3e+01     138.00    58586  207.3575  +38.8633
 10600  B3VLA 862                         3.20e+01  6.4e+00      69.00   -58586  207.3571  +38.8617

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