Complement to VIII/85A

Source 7C_042907.79+413209.00: 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  7C 042907.79+413209.00            1.96e+04  3.9e+03      70.20   17195 4   -0.46    5.33  068.1516  +41.6414
  178  3CR 119                           1.50e+04  3.0e+03     360.00   17195 4   -0.46    5.33  068.1546  +41.6533
  178  4C +41.13                         1.64e+04  4.9e+03     690.00   17195 4   -0.46    5.33  068.1508  +41.6433
  232  MY 042907.7+413822.8              1.74e+04  3.5e+03     150.00   17195 4   -0.46    5.33  068.1513  +41.6397
  325  WN B0429.1+4132                   1.77e+04  3.5e+03      12.00   17195 4   -0.46    5.33  068.1521  +41.6412
  365  TXS 0429+415                      1.65e+04  3.3e+03       6.00   17195 4   -0.46    5.33  068.1520  +41.6412
  408  B3 0429+415                       1.39e+04  2.8e+03      84.00   17195 4   -0.46    5.33  068.1529  +41.6403
 1400  NVSS J043236+413829               9.83e+03  2.0e+03      45.00   17195 4   -0.47    5.38  068.1517  +41.6414
 1400  WB 0429+4132                      7.57e+03  1.5e+03     120.00   17195 4   -0.46    5.33  068.1467  +41.6425
 1465  [P82] 0429+415                    8.60e+03  1.7e+03      25.80   17195 4   -0.46    5.33  068.1520  +41.6413
 2700  F3R 4626                          5.73e+03  1.1e+03     150.00   17195 4   -0.46    5.33  068.1425  +41.6361
 4850  87GB 042906.4+413212              4.30e+03  8.6e+02     138.00   17195 4   -0.46    5.33  068.1458  +41.6422
 4850  BWE 0429+4132                     4.30e+03  8.6e+02     138.00   17195 4   -0.51    5.47  068.1467  +41.6425
 4850  GB6 B0429+4132                    3.93e+03  7.9e+02     108.00   17195 4   -0.51    5.47  068.1504  +41.6417
 4885  [P82a] 0429+415                   3.70e+03  7.4e+02       6.00   17195 4   -0.47    5.38  068.1520  +41.6413
 8400  CLASS J043236.5037+413828.434     2.62e+03  5.2e+02       0.33   17195 4   -0.46    5.33  068.1521  +41.6412
 8400  JVAS J0432+416                    2.62e+03  5.2e+02       0.33   17195 4   -0.46    5.33  068.1521  +41.6412

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 J0432.6+4138                 1.46e+04  2.9e+03      79.98   -17195  068.1542  +41.6411
   151  7C 042907.79+413209.00            1.96e+04  3.9e+03      70.20    17195  068.1516  +41.6414
   178  3CR 119                           1.50e+04  3.0e+03     360.00    17195  068.1546  +41.6533
   178  4C +41.13                         1.64e+04  4.9e+03     690.00    17195  068.1508  +41.6433
   232  MY 042907.7+413822.8              1.74e+04  3.5e+03     150.00    17195  068.1513  +41.6397
   325  WN B0429.1+4132                   1.77e+04  3.5e+03      12.00    17195  068.1521  +41.6412
   325  WN B0429.4+4136                   1.84e+02  3.7e+01      12.00   -17195  068.2316  +41.7062
   365  TXS 0429+415                      1.65e+04  3.3e+03       6.00    17195  068.1520  +41.6412
   408  B3 0429+415                       1.39e+04  2.8e+03      84.00    17195  068.1529  +41.6403
  1400  NVSS J043236+413829               9.83e+03  2.0e+03      45.00    17195  068.1517  +41.6414
  1400  NVSS J043255+414220               5.58e+01  1.1e+01      45.00   -17195  068.2317  +41.7057
  1400  WB 0429+4132                      7.57e+03  1.5e+03     120.00    17195  068.1467  +41.6425
  2700  F3R 4626                          5.73e+03  1.1e+03     150.00    17195  068.1425  +41.6361
  4850  87GB 042906.4+413212              4.30e+03  8.6e+02     138.00    17195  068.1458  +41.6422
  4885  [P82a] 0429+415                   3.70e+03  7.4e+02       6.00    17195  068.1520  +41.6413
  8350  GPA1 160.89-4.28                  2.29e+03  4.6e+02     582.00   -17195  068.1425  +41.7406
  8350  GPA1 161.01-4.31                  1.27e+03  2.5e+02     582.00   -17195  068.2308  +41.6289
  8400  CLASS J043236.5037+413828.434     2.62e+03  5.2e+02       0.33    17195  068.1521  +41.6412

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