Complement to VIII/85A

Source BWE_0038-0159: 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 J0041.4-0143                 1.54e+04  3.1e+03      79.98    4002 0   -0.90    5.88  010.3581  -01.7208
   80  Cula 0038-019                     1.90e+04  3.8e+03     222.00    4002 0   -0.90    5.88  010.3613  -01.7219
  160  Culb 0038-019                     1.00e+04  2.0e+03     111.00    4002 0   -0.92    5.93  010.3613  -01.7219
  365  TXS 0038-019                      3.77e+03  7.5e+02       6.00    4002 0   -0.89    5.86  010.3583  -01.7206
  408  MRC 0038-019                      3.29e+03  6.6e+02     120.00    4002 0   -0.89    5.86  010.3592  -01.7197
 1400  NVSS J004126-014315               1.03e+03  2.1e+02      45.00    4002 0   -0.90    5.88  010.3583  -01.7208
 1400  WB 0038-0159                      1.42e+03  2.8e+02     120.00    4002 0   -0.89    5.85  010.3542  -01.7150
 2700  PKS J0041-0143                    6.20e+02  1.2e+02      60.00    4002 0   -0.90    5.88  010.3621  -01.7200
 4850  BWE 0038-0159                     4.16e+02  8.3e+01     138.00    4002 0   -0.89    5.85  010.3542  -01.7150
 4850  PMN J0041-0143                    3.51e+02  7.0e+01     168.00    4002 0   -0.89    5.85  010.3592  -01.7228

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  


   178  4C -02.04                         6.80e+03  2.0e+03     690.00    -4002  010.3588  -01.7433
   611  NAIC 0038-020                     2.37e+03  4.7e+02     756.00    -4002  010.3408  -01.7258
  1400  FIRST J004123.4-014201            6.00e-01  2.0e-01       5.00    -4002  010.3476  -01.7003
  1400  FIRST J004125.4-014030            1.70e+00  3.0e-01       5.00    -4002  010.3562  -01.6752
  1400  FIRST J004128.3-014416            1.90e+00  4.0e-01       5.00    -4002  010.3682  -01.7378
  4850  PMN J0041-0143                    3.51e+02  7.0e+01     168.00     4002  010.3592  -01.7228

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