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| author | tlatorre <tlatorre@uchicago.edu> | 2018-09-11 10:25:28 -0500 |
|---|---|---|
| committer | tlatorre <tlatorre@uchicago.edu> | 2018-09-11 10:25:28 -0500 |
| commit | d70984de03adf3ceb37734b700426d0f1ededd7f (patch) | |
| tree | a76882e9c10a1b84ae523901786f7cb3fdab29f0 /src/optics.h | |
| parent | ebe4b59376622009818ffb96f109221571e33dfb (diff) | |
| download | sddm-d70984de03adf3ceb37734b700426d0f1ededd7f.tar.gz sddm-d70984de03adf3ceb37734b700426d0f1ededd7f.tar.bz2 sddm-d70984de03adf3ceb37734b700426d0f1ededd7f.zip | |
add absorption length
This commit adds the absorption length to the likelihood calculation. For now
I'm just using a single number independent of wavelength. I should update this
in the future to actually use the absorption lengths as measured by SNO and
then calculate an overall absorption length weighted by the Cerenkov spectrum
and the PMT quantum efficiency.
Diffstat (limited to 'src/optics.h')
| -rw-r--r-- | src/optics.h | 1 |
1 files changed, 1 insertions, 0 deletions
diff --git a/src/optics.h b/src/optics.h index e2df659..5a6dec9 100644 --- a/src/optics.h +++ b/src/optics.h @@ -1,6 +1,7 @@ #ifndef OPTICS_H #define OPTICS_H +double get_absorption_length_snoman_d2o(double wavelength); double get_index(double p, double wavelength, double T); double get_index_snoman_h2o(double wavelength); double get_index_snoman_d2o(double wavelength); |