Complement to VIII/85A

Source WB_1111+4053: 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  


  178  3CR 254                           1.90e+04  3.8e+03     360.00  106476 0   -1.03    6.72  168.6654  +40.6267
  178  4C +40.28                         2.17e+04  6.5e+03     690.00  106476 0   -1.03    6.72  168.6587  +40.6217
  232  MY 111153.2+403714.2              1.95e+04  3.9e+03     150.00  106476 0   -1.08    6.85  168.6608  +40.6206
  325  WN B1111.8+4053                   1.40e+04  2.8e+03      12.00  106476 0   -1.08    6.85  168.6607  +40.6206
  365  TXS 1111+408                      1.26e+04  2.5e+03       6.00  106476 0   -1.03    6.72  168.6603  +40.6223
  408  B3 1111+408                       1.09e+04  2.2e+03      84.00  106476 0   -1.08    6.85  168.6612  +40.6242
 1400  NVSS J111438+403720               3.13e+03  6.3e+02      45.00  106476 0   -1.08    6.85  168.6601  +40.6224
 1400  WB 1111+4053                      3.08e+03  6.2e+02     120.00  106476 0   -1.08    6.85  168.6592  +40.6200
 4850  87GB 111152.7+405333              7.59e+02  1.5e+02     138.00  106476 0   -1.03    6.72  168.6587  +40.6200
 4850  BWE 1111+4053                     6.70e+02  1.3e+02     138.00  106476 0   -1.03    6.72  168.6592  +40.6200
 4850  GB6 B1111+4053                    6.88e+02  1.4e+02     108.00  106476 0   -1.03    6.72  168.6625  +40.6200

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 J1114.6+4037                 5.12e+04  1.0e+04      79.98  -106476  168.6612  +40.6225
   151  6C 111153+405339                  2.78e+04  5.6e+03     252.00  -106476  168.6600  +40.6217
   151  7C 111150.79+405432.00            3.96e+03  7.9e+02      70.20  -106476  168.6508  +40.6364
   151  7C 111153.20+405339.00            2.76e+04  5.5e+03      70.20  -106476  168.6608  +40.6217
   159  3C 254                            2.15e+04  4.3e+03     600.00  -106476  168.6683  +40.6933
   178  4C +40.28                         2.17e+04  6.5e+03     690.00   106476  168.6587  +40.6217
   232  MY 111153.2+403714.2              1.95e+04  3.9e+03     150.00   106476  168.6608  +40.6206
   325  WN B1111.8+4053                   1.40e+04  2.8e+03      12.00   106476  168.6607  +40.6206
   365  TXS 1111+408                      1.26e+04  2.5e+03       6.00   106476  168.6603  +40.6223
   408  B3 1111+408                       1.09e+04  2.2e+03      84.00   106476  168.6612  +40.6242
   408  B3 1112+408                       2.10e+02  4.2e+01      84.00  -106476  168.7092  +40.5369
  1400  FIRST J111437.7+403723            1.03e+03  2.1e+02       5.00  -106476  168.6573  +40.6231
  1400  FIRST J111438.8+403719            2.00e+03  4.0e+02       5.00  -106476  168.6617  +40.6220
  1400  FIRST J111440.3+404226            1.90e+00  4.0e-01       5.00  -106476  168.6682  +40.7075
  1400  FIRST J111444.7+403717            3.30e+00  7.0e-01       5.00  -106476  168.6864  +40.6216
  1400  FIRST J111447.2+404004            2.60e+00  5.0e-01       5.00  -106476  168.6967  +40.6678
  1400  FIRST J111452.2+403216            3.00e+00  6.0e-01       5.00  -106476  168.7179  +40.5379
  1400  FIRST J111453.2+403213            6.90e+00  1.4e+00       5.00  -106476  168.7217  +40.5372
  1400  NVSS J111438+403720               3.13e+03  6.3e+02      45.00   106476  168.6601  +40.6224
  4730  B3a 1111+408                      7.69e+02  1.5e+02     168.00  -106476  168.6612  +40.6242
  4850  87GB 111152.7+405333              7.59e+02  1.5e+02     138.00   106476  168.6587  +40.6200
  4885  RGB 1114+406A                     6.88e+02  1.4e+02       4.02  -106476  168.6571  +40.6231
  4885  RGB 1114+406B                     6.88e+02  1.4e+02       4.02  -106476  168.6618  +40.6221
  5000  RGB6 J1114.6+4037                 7.96e+02  1.6e+02     144.00  -106476  168.6592  +40.6200
 10600  B3VLA 645                         2.49e+02  5.0e+01      69.00  -106476  168.6600  +40.6222

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