We provide the radial profiles for 22/25 clusters as they were published in Kamann et al. (2017,  arxiv:1710.07257). We kindly ask you to cite this paper when using the data.

The data set for each cluster is provided as a plain csv-file, containing one radial bin per line.

Data

NGC 104 NGC 362 NGC 1851 NGC 2808 NGC 3201
NGC 5139 NGC 5904 NGC 6093 NGC 6121 NGC 6254
NGC 6266 NGC 6293 NGC 6388 NGC 6441 NGC 6522
NGC 6541 NGC 6656 NGC 6681 NGC 6752 NGC 7078
NGC 7089 NGC 7099      

Each file contains the following columns:

  • logr mean - The mean distance of the stars to the cluster centre (in log[arcseconds]).
  • logr min - The lower edge of the radial bin (in log[arcseconds])
  • logr max - The upper edge of the radial bin (in log[arcseconds])
  • theta0 - The maximum-likelihood solution for the axis angle of the rotation field (in radians, north through east)
  • theta0 mc low/median/high - The 16%/50%/86% percentiles of the axis angle distribution obtained in the MCMC analysis (in radians, north through east)
  • v_rot - The maximum-likelihood solution for the rotation velocity (in km/s)
  • v_rot mc low/median/high - The 16%/50%/86% percentiles of the rotation velocity distribution obtained in the MCMC analysis (in km/s)
  • v_disp - The maximum-likelihood solution for the velocity dispersion (in km/s)
  • v_disp mc low/median/high - The 16%/50%/86% percentiles of the velocity dispersion distribution obtained in the MCMC analysis (in km/s)
  • Effective mass - The variance-weighted mean mass of the stars that contribute to the kinematics analysis

 

Targets

Publications

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