Complement to VIII/104

Source PMN_J0134-3629: 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 1 column 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/104/spectra
Post annotation 		SPECFIND V3.0 Catalog of radio continuum spectra (Stein+, 2021) [ReadMe+ftp]
2021A&A...655A..17S

The parameters of the radio spectra[image] (1658207 rows)		img(gal)
start AladinLite 
  nu   Name                                   S(nu)       e         beam        Seq      a       b      RAJ2000   DEJ2000
 MHz                                           mJy       mJy       arcsec                      [mJy]      deg       deg  


   38  8C 110623+615524                      2.20e+03  4.4e+02      270.0000  144298   -0.80     4.61  167.3542  +61.6522
   74  VLSSr J110931.1+613945                8.80e+02  1.8e+02       75.0000  144298   -0.71     4.32  167.3797  +61.6628
  150  TGSSADR J110929.7+613950              7.15e+02  1.4e+02       25.0020  144298   -0.79     4.58  167.3741  +61.6640
  151  6C 110627+615604                      6.80e+02  1.4e+02      252.0000  144298   -0.80     4.61  167.3708  +61.6633
  151  7C 110628.89+615606.00                7.81e+02  1.6e+02       70.2000  144298   -0.71     4.32  167.3779  +61.6636
  325  WN B1106.4+6156                       4.12e+02  8.2e+01       12.0000  144298   -0.79     4.58  167.3742  +61.6638
  365  TXS 1106+619                          4.06e+02  8.1e+01        6.0000  144298   -0.79     4.58  167.3749  +61.6637
 1400  NVSS J110929+613951                   1.25e+02  2.5e+01       45.0000  144298   -0.79     4.58  167.3744  +61.6644
 4850  87GB 110627.3+615552                  4.87e+01  9.7e+00      138.0000  144298   -0.80     4.61  167.3713  +61.6600
 4850  BWE 1106+6156                         4.10e+01  8.2e+00      138.0000  144298   -0.79     4.59  167.3738  +61.6622
 4850  GB6 B1106+6156                        4.00e+01  8.0e+00      108.0000  144298   -0.79     4.59  167.3812  +61.6631

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/104/waste
Post annotation 		SPECFIND V3.0 Catalog of radio continuum spectra (Stein+, 2021) [ReadMe+ftp]
2021A&A...655A..17S

Source parameters based on positional cross-id[spectrum] (3570814 rows)		img(gal)
start AladinLite 
  nu    Name                                S(nu)       e         beam         Seq     RAJ2000   DEJ2000
  MHz                                        mJy       mJy       arcsec                  deg       deg  


   145  [JAP2011] J23.55-36.52             2.61e+04  5.2e+03     1560.0000   -144298  023.5500  -36.5200
  1400  NVSS J013419-362615                5.90e+01  1.2e+01       45.0000   -144298  023.5833  -36.4376
  2307  SPASS J013356-362905               5.85e+03  1.2e+03      645.0000   -144298  023.4862  -36.4848
  4850  PMN J0134-3629                     1.51e+03  3.0e+02      168.0000   -144298  023.5500  -36.4872

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