Complement to VIII/85A

Source BWE_1043+3714: 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 104321+371414                  2.81e+03  5.6e+02     252.00   42370 4   -1.12    5.93  161.5483  +36.9736
  151  7C 104322.00+371433.00            2.54e+03  5.1e+02      70.20   42370 4   -1.12    5.91  161.5500  +36.9789
  178  4C +37.28                         2.50e+03  7.5e+02     690.00   42370 4   -1.12    5.93  161.5508  +37.0650
  232  MY 104322.1+365821.3              1.86e+03  3.7e+02     150.00   42370 4   -1.12    5.91  161.5504  +36.9726
  325  WN B1043.3+3714                   1.29e+03  2.6e+02      12.00   42370 4   -1.12    5.91  161.5498  +36.9792
  365  TXS 1043+372                      1.18e+03  2.4e+02       6.00   42370 4   -1.12    5.91  161.5495  +36.9791
  408  B2.3 1043+37A                     1.10e+03  2.2e+02       0.00   42370 4   -1.11    5.89  161.5521  +36.9717
 1400  FIRST J104611.9+365844            2.48e+02  5.0e+01       5.00   42370 4   -1.12    5.91  161.5496  +36.9792
 1400  NVSS J104611+365845               2.64e+02  5.3e+01      45.00   42370 4   -1.12    5.91  161.5497  +36.9792
 1400  WB 1043+3714                      2.62e+02  5.2e+01     120.00   42370 4   -1.12    5.91  161.5529  +36.9775
 1465  [RLM94] 1043+372A                 2.28e+02  4.6e+01       4.50   42370 4   -1.12    5.91  161.5496  +36.9786
 4850  87GB 104322.4+371423              6.50e+01  1.3e+01     138.00   42370 4   -1.09    5.86  161.5517  +36.9764
 4850  BWE 1043+3714                     5.60e+01  1.1e+01     138.00   42370 4   -1.12    5.91  161.5529  +36.9775
 4850  GB6 B1043+3714                    6.22e+01  1.2e+01     108.00   42370 4   -1.09    5.86  161.5488  +36.9742

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 J1046.1+3658                 3.01e+03  6.0e+02      79.98   -42370  161.5496  +36.9789
   151  6C 104321+371414                  2.81e+03  5.6e+02     252.00    42370  161.5483  +36.9736
   151  7C 104322.00+371433.00            2.54e+03  5.1e+02      70.20    42370  161.5500  +36.9789
   178  4C +37.28                         2.50e+03  7.5e+02     690.00    42370  161.5508  +37.0650
   232  MY 104322.1+365821.3              1.86e+03  3.7e+02     150.00    42370  161.5504  +36.9726
   325  WN B1043.3+3714                   1.29e+03  2.6e+02      12.00    42370  161.5498  +36.9792
   365  TXS 1043+372                      1.18e+03  2.4e+02       6.00    42370  161.5495  +36.9791
   408  B2.3 1043+37A                     1.10e+03  2.2e+02       0.00    42370  161.5521  +36.9717
  1400  FIRST J104606.5+365658            3.00e+00  6.0e-01       5.00   -42370  161.5272  +36.9495
  1400  FIRST J104607.2+365711            6.60e+00  1.3e+00       5.00   -42370  161.5302  +36.9533
  1400  FIRST J104607.4+365839            2.80e+00  6.0e-01       5.00   -42370  161.5309  +36.9776
  1400  FIRST J104608.1+365732            4.00e+00  8.0e-01       5.00   -42370  161.5339  +36.9590
  1400  FIRST J104609.1+365757            2.10e+00  4.0e-01       5.00   -42370  161.5383  +36.9661
  1400  FIRST J104611.9+365844            2.48e+02  5.0e+01       5.00    42370  161.5496  +36.9792
  1400  FIRST J104616.5+365850            3.20e+00  6.0e-01       5.00   -42370  161.5687  +36.9808
  1400  FIRST J104617.3+370032            4.70e+00  9.0e-01       5.00   -42370  161.5723  +37.0091
  1400  FIRST J104620.5+365846            1.16e+01  2.3e+00       5.00   -42370  161.5856  +36.9796
  1400  NVSS J104611+365845               2.64e+02  5.3e+01      45.00    42370  161.5497  +36.9792
  1400  WB 1043+3714                      2.62e+02  5.2e+01     120.00    42370  161.5529  +36.9775
  1465  [RLM94] 1043+372A                 2.28e+02  4.6e+01       4.50    42370  161.5496  +36.9786
  1465  [RLM94] 1043+372B                 5.70e+01  1.1e+01       4.50   -42370  161.5495  +36.9796
  4850  GB6 B1043+3714                    6.22e+01  1.2e+01     108.00    42370  161.5488  +36.9742

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