Complement to VIII/85A

Source GB6_B0110+4010: 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  


  232  MY 011026.9+402608.0              1.16e+03  2.3e+02     150.00    2620 0   -0.58    4.55  018.3254  +40.4356
  408  B2.3 0110+40                      1.25e+03  2.5e+02       0.00    2620 0   -0.62    4.68  018.3225  +40.4367
  408  B3 0110+401                       1.08e+03  2.2e+02      84.00    2620 0   -0.63    4.69  018.3233  +40.4361
 1400  NVSS J011317+402613               5.46e+02  1.1e+02      45.00    2620 0   -0.63    4.70  018.3242  +40.4370
 1400  WB 0110+4010                      6.22e+02  1.2e+02     120.00    2620 0   -0.63    4.69  018.3229  +40.4383
 4850  87GB 011026.2+401024              2.83e+02  5.7e+01     138.00    2620 0   -0.63    4.69  018.3225  +40.4381
 4850  GB6 B0110+4010                    2.66e+02  5.3e+01     108.00    2620 0   -0.63    4.69  018.3225  +40.4353
 4860  [FPD2001b]a 24                    2.40e+02  4.8e+01       0.40    2620 0   -0.62    4.68  018.3239  +40.4369
 4860  [FPD2001b]a 25                    2.40e+02  4.8e+01       0.40    2620 0   -0.62    4.68  018.3239  +40.4371
 8400  CLASS J011317.7774+402613.131     1.42e+02  2.8e+01       0.33    2620 0   -0.63    4.70  018.3240  +40.4370
 8400  CLASS J011317.7781+402613.118     1.26e+02  2.5e+01       0.33    2620 0   -0.63    4.69  018.3240  +40.4370
 8400  JVAS J0113+404                    1.68e+02  3.4e+01       0.33    2620 0   -0.63    4.69  018.3241  +40.4370

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 J0113.3+4026                 3.02e+03  6.0e+02      79.98    -2620  018.3251  +40.4378
   232  MY 011026.9+402608.0              1.16e+03  2.3e+02     150.00     2620  018.3254  +40.4356
   325  WN B0110.4+4010                   1.30e+03  2.6e+02      12.00    -2620  018.3241  +40.4365
   365  TXS 0110+401                      1.21e+03  2.4e+02       6.00    -2620  018.3242  +40.4371
   408  B2.3 0110+40                      1.25e+03  2.5e+02       0.00     2620  018.3225  +40.4367
   408  B3 0110+401                       1.08e+03  2.2e+02      84.00     2620  018.3233  +40.4361
  1400  WB 0110+4010                      6.22e+02  1.2e+02     120.00     2620  018.3229  +40.4383
  4730  B3a 0110+401                      2.53e+02  5.1e+01     168.00    -2620  018.3235  +40.4364
  4850  87GB 011026.2+401024              2.83e+02  5.7e+01     138.00     2620  018.3225  +40.4381
  4850  BWE 0110+4010                     2.78e+02  5.6e+01     138.00    -2620  018.3229  +40.4383
  4850  GB6 B0110+4010                    2.66e+02  5.3e+01     108.00     2620  018.3225  +40.4353
  4850  MITG J011315+4025                 2.25e+02  4.5e+01     258.00    -2620  018.3158  +40.4306
  4860  [FPD2001b]a 24                    2.40e+02  4.8e+01       0.40     2620  018.3239  +40.4369
  4860  [FPD2001b]a 25                    2.40e+02  4.8e+01       0.40     2620  018.3239  +40.4371
  4860  [FPD2001b]a 26                    2.40e+01  4.8e+00       0.40    -2620  018.3238  +40.4371
  8400  CLASS J011317.7627+402612.664     6.26e+01  1.2e+01       0.33    -2620  018.3240  +40.4368
  8400  CLASS J011317.7636+402612.664     4.43e+01  8.9e+00       0.33    -2620  018.3240  +40.4368
  8400  CLASS J011317.7645+402612.609     3.59e+01  7.2e+00       0.33    -2620  018.3240  +40.4368
  8400  CLASS J011317.7747+402613.035     8.16e+01  1.6e+01       0.33    -2620  018.3240  +40.4370
  8400  CLASS J011317.7781+402613.118     1.26e+02  2.5e+01       0.33     2620  018.3240  +40.4370
  8400  CLASS J011317.7830+402613.105     4.51e+01  9.0e+00       0.33    -2620  018.3241  +40.4370
  8460  [FPD2001b]b 24                    4.12e+01  8.2e+00       0.20    -2620  018.3239  +40.4369
  8460  [FPD2001b]b 25                    1.23e+02  2.5e+01       0.20    -2620  018.3239  +40.4371
 10600  B3VLA 111                         1.44e+02  2.9e+01      69.00    -2620  018.3238  +40.4367

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