Complement to VIII/85A

Source 87GB_030842.8+251846: 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 J0311.6+2530                 4.31e+03  8.6e+02      79.98    9823 1   -0.55    4.66  047.9200  +25.5012
  365  TXS 0308+253                      2.07e+03  4.1e+02       6.00    9823 1   -0.55    4.66  047.9202  +25.5027
 1400  NVSS J031140+253009               7.98e+02  1.6e+02      45.00    9823 1   -0.57    4.71  047.9203  +25.5026
 1400  WB 0308+2518                      8.54e+02  1.7e+02     120.00    9823 1   -0.57    4.71  047.9171  +25.5006
 2700  PKS J0311+2529                    6.00e+02  1.2e+02      60.00    9823 1   -0.57    4.71  047.9179  +25.4989
 4850  87GB 030842.8+251846              3.53e+02  7.1e+01     138.00    9823 1   -0.55    4.66  047.9167  +25.5006
 4850  BWE 0308+2518                     2.88e+02  5.8e+01     138.00    9823 1   -0.80    5.43  047.9171  +25.5006
 4850  GB6 B0308+2518                    3.48e+02  7.0e+01     108.00    9823 1   -0.55    4.66  047.9200  +25.5022
 4850  MITG J031141+2529                 3.26e+02  6.5e+01     258.00    9823 1   -0.55    4.66  047.9225  +25.4950

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  


    80  Cula 0308+252                     9.00e+03  1.8e+03     222.00    -9823  047.9308  +25.4683
   160  Culb 0308+252                     3.50e+03  7.0e+02     111.00    -9823  047.9308  +25.4683
   178  4C +25.11                         2.40e+03  7.2e+02     690.00    -9823  047.9204  +25.4650
   408  B2.2 0308+25                      2.03e+03  4.1e+02       0.00    -9823  047.9171  +25.5083
  1400  NVSS J031135+252846               1.64e+01  3.3e+00      45.00    -9823  047.8983  +25.4795
  4850  87GB 030842.8+251846              3.53e+02  7.1e+01     138.00     9823  047.9167  +25.5006
  4850  MITG J031141+2529                 3.26e+02  6.5e+01     258.00     9823  047.9225  +25.4950

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