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new release (develop --> master)

Leo Michel-Dansac requested to merge develop into master

New features:

  • New transitions and species (FeII lines -- see mclya/rascas!30 ; SiII_1260 -- see mclya/rascas!33)
  • New gas composition modules -- see mclya/rascas!30, mclya/rascas!33, mclya/rascas!42
  • New Voigt module (with the three approximations) -- see mclya/rascas!31
  • New code LyaPhotonsFromGas (from Jeremy Blaizot) -- see mclya/rascas!41
  • New method for the emission of photon packets: no longer use pre-computed PhotTables in Python; instead, fluxes, luminosities, and weights are computed directly in Fortran from SSP/SED library (new module_ssp_lib.f90) -- see mclya/rascas!41
  • New scheme for selecting cells in domain ; it now selects all cells that may intersect the domain ; this allows to use the same size for the computational domain and the data domain. -- see mclya/rascas!42

Optimizations:

  • Add an OpenMP reader for star particles -- see mclya/rascas!41
  • Faster sampling method in PhotonsFromStars (thanks to Harley Katz) -- see mclya/rascas!41
  • Some code optimizations for better performance -- see mclya/rascas!34

Corrections and updates:

  • Update of the atomic data: all atomic data are now from the NIST database -- see mclya/rascas!35
  • Correct positions for periodic boundaries everywhere -- see mclya/rascas!38
  • Update the phase function inversion for HI (core and wing) -- see mclya/rascas!37
  • Correction of the definition of the MPI type photon -- see mclya/rascas!40
  • Improve and homogenize verbose, logs, variable names, etc. -- see mclya/rascas!36, mclya/rascas!42
Edited by Leo Michel-Dansac

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