1. 06 Nov, 2018 1 commit
  2. 18 Sep, 2018 2 commits
  3. 16 Feb, 2018 3 commits
  4. 15 Jan, 2018 1 commit
    • Médéric Boquien's avatar
      Fν was computed by calculating Fλ and then converting to Fν, which led to... · d963067f
      Médéric Boquien authored
      Fν was computed by calculating Fλ and then converting to Fν, which led to typical differences in fluxes of typically 1-2% and a bit more for a handful of pathological filters. Now Fν is computed directly and a bit faster. At the same time rather than computing an effective wavelength (which was more a mean wavelength), we compute the pivot wavelength, which is more appropriate when converting between Fν and Fλ.
      d963067f
  5. 31 Oct, 2017 2 commits
  6. 25 Oct, 2017 1 commit
  7. 19 Oct, 2017 1 commit
  8. 18 Sep, 2017 3 commits
  9. 10 Feb, 2017 1 commit
  10. 03 Feb, 2017 1 commit
  11. 02 Feb, 2017 1 commit
  12. 28 Dec, 2016 1 commit
  13. 23 Dec, 2016 1 commit
  14. 22 Dec, 2016 1 commit
  15. 21 Dec, 2016 2 commits
  16. 16 Dec, 2016 1 commit
  17. 06 Sep, 2016 1 commit
    • Yannick Roehlly's avatar
      Update WFCAM filters · 07e4b43d
      Yannick Roehlly authored
      The WFCAM Ks filter does not exist.
      The filters J, and Y were wrong.
      Add H, K, and Z filters.
      07e4b43d
  18. 04 Dec, 2015 1 commit
  19. 02 Nov, 2015 1 commit
  20. 15 Oct, 2015 2 commits
  21. 14 Oct, 2015 2 commits
  22. 05 Oct, 2015 1 commit
  23. 04 Oct, 2015 1 commit
  24. 28 Sep, 2015 1 commit
    • 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
  25. 20 Sep, 2015 2 commits
  26. 31 Aug, 2015 1 commit
  27. 25 Aug, 2015 1 commit
  28. 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
  29. 23 Jul, 2015 2 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