1. 16 Oct, 2015 2 commits
  2. 15 Oct, 2015 1 commit
  3. 14 Oct, 2015 1 commit
  4. 13 Oct, 2015 1 commit
  5. 12 Oct, 2015 3 commits
  6. 11 Oct, 2015 5 commits
  7. 10 Oct, 2015 1 commit
  8. 08 Oct, 2015 1 commit
    • Médéric Boquien's avatar
      Computing the parameters and their uncertainties through the histogram of the... · e57cb6e6
      Médéric Boquien authored
      Computing the parameters and their uncertainties through the histogram of the PDF makes the code more complex and can introduce biases in some cases. This patch moves the computation of the histograms to the function that saves them onto the disk. In parallel the estimated value of the parameters and the corresponding uncertainties are simply computed from the weighted mean and standard deviation of the models that are at least 0.1% as likely as the best model to reproduce the observations.
      e57cb6e6
  9. 06 Oct, 2015 4 commits
  10. 05 Oct, 2015 5 commits
  11. 04 Oct, 2015 3 commits
  12. 02 Oct, 2015 1 commit
    • Yannick Roehlly's avatar
      Add flux computation to "param" module · 4b2d9012
      Yannick Roehlly authored
      Add the possibility to compute some fluxes in the "param" module to add
      them to the SED info dictionary.  This can be used for instance to
      compute probability distribution of fluxes during an analysis.
      4b2d9012
  13. 28 Sep, 2015 2 commits
    • Yannick Roehlly's avatar
      Correct error handling · d41e1401
      Yannick Roehlly authored
      When the error column for a flux was present in the observation table
      but not in the used column list (when the user prefers to use a default
      error instead of the real one), the error on the flux was set to 0.
      d41e1401
    • Yannick Roehlly's avatar
      Pseudo filter for Lyman continuum · 33d6870a
      Yannick Roehlly authored
      Addition of a pseudo filter to compute the flux in the Lyman continuum.
      This is a box function taking everything between 91 Å and 911 Å.
      
      NOTE: This filter was made for the BC03 SSP which begin at 91 Å. It
            can't be used if the spectrum is redshifted as the filter
            wavelengths will then be outside of the SED ones.
      33d6870a
  14. 25 Sep, 2015 1 commit
  15. 20 Sep, 2015 7 commits
  16. 19 Sep, 2015 1 commit
  17. 10 Sep, 2015 1 commit
    • Médéric Boquien's avatar
      Ensure that the .fnu @property returns a result even if the redshifting module... · cb56b290
      Médéric Boquien authored
      Ensure that the .fnu @property returns a result even if the redshifting module has not been applied. By default in that case we assume a distance of 10 parsecs. Note that as the redshifting module is mandatory (it is needed to apply the IGM absorption, which has a small effect even at z=0 with this formula), it should not happen. Issue found by Yannick Roehlly.
      cb56b290