1. 26 Aug, 2015 3 commits
  2. 25 Aug, 2015 4 commits
  3. 07 Aug, 2015 1 commit
  4. 31 Jul, 2015 2 commits
    • BURGARELLA Denis's avatar
      Fake parameter for param module · 9a3d7941
      BURGARELLA Denis authored
      For now, CIGALE does not work with a parameterless module, so we use
      a fake one.
      9a3d7941
    • BURGARELLA Denis's avatar
      New SED creation modules · 20f67dd5
      BURGARELLA Denis authored
      - mbb: modified black body
      - param: parameterless module to compute some parameters and add them to
        the information dictionary
      - sfhcomb_constant and sfhcomb_delayed: two star formation histories
      20f67dd5
  5. 24 Jul, 2015 1 commit
    • Yannick Roehlly's avatar
      PSEUDO filters must not be normalised · e9487032
      Yannick Roehlly authored
      The pseudo filters used to compute (pseudo) line fluxes must not be
      normalised to 1. Also, we set their effective wavelength to the mean
      wavelength of the positive part.
      e9487032
  6. 23 Jul, 2015 4 commits
    • Yannick Roehlly's avatar
      Correction to the pseudo filters · 4add16f3
      Yannick Roehlly authored
      The wavelengths must be in angstrom.
      4add16f3
    • Yannick Roehlly's avatar
      New pseudo filters to compute line fluxes · 095ef623
      Yannick Roehlly authored
      Addition of pseudo filters used to compute de fluxes in some lines.
      They are composed of a positive part (normalised to 1) above the line
      and two negative part (of the same total area) on each side used to
      remove the continuum.
      
      The PSEUDO_D4000 pseudo filter measures the difference (not the ratio)
      of the 4000 Å break.
      095ef623
    • Yannick Roehlly's avatar
      SFH_quenching module · a303838b
      Yannick Roehlly authored
      Addition of a new module performing a quench on the star formation
      history.  We must change a little the SED object to allow the
      modification of the SED.
      a303838b
    • Yannick Roehlly's avatar
      Buat 2008 SFH module · 2fac3c85
      Yannick Roehlly authored
      Addition of a new module to compute a star formation history as
      described in Buat et al. 2008.
      2fac3c85
  7. 16 Jul, 2015 2 commits
  8. 15 Jul, 2015 2 commits
  9. 26 May, 2015 1 commit
  10. 25 May, 2015 1 commit
  11. 24 May, 2015 3 commits
  12. 22 May, 2015 3 commits
  13. 21 May, 2015 2 commits
    • Médéric Boquien's avatar
      Implement a cache for the computation of the optimal grid when merging two... · 3eb0c388
      Médéric Boquien authored
      Implement a cache for the computation of the optimal grid when merging two grids. As the best_grid() function takes numpy arrays as arguments, it makes caching difficult as they are not hashable. To solve the problem we define a helper function to do the memoisation based on the size, min, and max values of each of the input arrays.
      3eb0c388
    • Médéric Boquien's avatar
      Implement a cache for the filters to compute the fluxes. Rather than passing... · 38e7f35b
      Médéric Boquien authored
      Implement a cache for the filters to compute the fluxes. Rather than passing the transmission table as an argument to compute_fnu(), which makes caching difficult and/or slow to compute the hash, we rather pass the filter name. Then the SED object fetches the filter from the database and resamples it on the optimal wavelength grid. The result is stored in cache to avoid carrying out this operation repeatedly.
      38e7f35b
  14. 20 May, 2015 9 commits
  15. 19 May, 2015 2 commits