1. 29 Aug, 2015 5 commits
  2. 28 Aug, 2015 6 commits
  3. 27 Aug, 2015 2 commits
    • Médéric Boquien's avatar
      As python evaluates expressions from the left to the right, put the vector in... · 8f51e634
      Médéric Boquien authored
      As python evaluates expressions from the left to the right, put the vector in the rightmost position so that we do not multiply it with a scalar several times.
      8f51e634
    • Médéric Boquien's avatar
      When computing the flux in filters, np.trapz() become the bottleneck of the... · ce4d814d
      Médéric Boquien authored
      When computing the flux in filters, np.trapz() become the bottleneck of the code. A large part of the time is spent on safeguards and on operations for nD arrays. However in our specific case we only have 1D arrays. Also we can cache some computed variables, for instance dx which only depends on the wavelength sampling. We do that employing the same key that is used for caching the best sampling of each filter in compute_fnu(). That way the caches are consistent. The key is based on the size of the wavelength grid, the name of the filter, and the redshift.
      ce4d814d
  4. 26 Aug, 2015 4 commits
  5. 25 Aug, 2015 4 commits
  6. 07 Aug, 2015 1 commit
  7. 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
  8. 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
  9. 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
  10. 16 Jul, 2015 2 commits
  11. 15 Jul, 2015 2 commits
  12. 26 May, 2015 1 commit
  13. 25 May, 2015 1 commit
  14. 24 May, 2015 3 commits
  15. 22 May, 2015 2 commits