new release (develop --> 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