1. 24 Apr, 2015 1 commit
  2. 10 Nov, 2014 4 commits
  3. 14 Oct, 2014 1 commit
  4. 22 Aug, 2014 2 commits
  5. 21 Aug, 2014 2 commits
  6. 29 Mar, 2014 1 commit
  7. 28 Mar, 2014 2 commits
  8. 12 Mar, 2014 1 commit
  9. 11 Mar, 2014 2 commits
  10. 03 Mar, 2014 2 commits
  11. 28 Feb, 2014 1 commit
  12. 20 Feb, 2014 1 commit
  13. 18 Feb, 2014 2 commits
  14. 29 Jan, 2014 1 commit
    • Yannick Roehlly's avatar
      Change how redshit and fluxes are managed · 2f29f425
      Yannick Roehlly authored
      Now the redshift is an attribute of the SED.
      
      The SED.compute_fnu() no longuer takes redshift and apply_redshift
      arguments as the SED is supposed to be redshifted.
      
      The SED.lambda_fnu() method was converted to the SED.fnu property
      returning th Fν flux density at each wavelength of the wavelength grid.
      2f29f425
  15. 11 Jan, 2014 1 commit
    • Yannick Roehlly's avatar
      Add AUTHORS.rst file · f9feb391
      Yannick Roehlly authored
      Remove the author email addresses from the source files and add a AUTHORS.rst
      file with the addresses and current affiliation to make it easier to update
      the information.
      
      Also, give copyright to the University of Cambridge and the University of
      Crete for code developed by authors working there.
      f9feb391
  16. 29 Nov, 2013 1 commit
  17. 17 Sep, 2013 1 commit
  18. 16 Sep, 2013 2 commits
  19. 08 Jul, 2013 1 commit
  20. 05 Jul, 2013 1 commit
  21. 02 Jul, 2013 3 commits
  22. 01 Jul, 2013 1 commit
    • Yannick Roehlly's avatar
      Correct the redshifting · 08c5c6b4
      Yannick Roehlly authored
      The redshifting also lower the fluxes (that's different from the
      cosmological dimming).
      Also, simplify some methods.
      08c5c6b4
  23. 17 Jun, 2013 2 commits
    • Yannick Roehlly's avatar
      Add a lines property to the SED · dd430087
      Yannick Roehlly authored
      It's a dictionnary to hold the spectral lines associated with the SED.
      We use a disctionnary to be able to differentiate several sets of lines
      (e.g. lines from old and young populations).
      
      TODO: Complete the code to add the line contributions to the integrated flux.
      dd430087
    • Yannick Roehlly's avatar
      Simplify the SED class · 84ec7cd1
      Yannick Roehlly authored
      Rename lumin_contributions to luminosities and use a 2 axis numpy array
      instead of a list of arrays. This should accelerate some operations.
      
      The star formation history is now stored in its own property.
      TODO: maybe automatically add age and instantaneous SFR to the info dictionnary when setting the SFH.
      84ec7cd1
  24. 29 Apr, 2013 2 commits
  25. 03 Apr, 2013 1 commit
  26. 06 Feb, 2013 1 commit