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| author | tlatorre <tlatorre@uchicago.edu> | 2020-11-03 08:10:42 -0600 |
|---|---|---|
| committer | tlatorre <tlatorre@uchicago.edu> | 2020-11-03 08:10:42 -0600 |
| commit | 3958f04ff6202f0f9f137285fbebdef399b8851d (patch) | |
| tree | 5a52a9c6ec7cf02905e941b9320e994dcb7a3ac4 /utils/chi2 | |
| parent | 220377d85d8cf71d37a47b160ff71bdfadce8f38 (diff) | |
| download | sddm-3958f04ff6202f0f9f137285fbebdef399b8851d.tar.gz sddm-3958f04ff6202f0f9f137285fbebdef399b8851d.tar.bz2 sddm-3958f04ff6202f0f9f137285fbebdef399b8851d.zip | |
initial commit of a script to do the dark matter search
Diffstat (limited to 'utils/chi2')
| -rwxr-xr-x | utils/chi2 | 2 |
1 files changed, 0 insertions, 2 deletions
@@ -68,8 +68,6 @@ FIT_PARS = [ # at that energy level we don't see anything which leads us to expect a major # difference. To be conservative, and because I don't think it really affects # the analysis at all, I'll leave the uncertainty here at 10% anyways. -# - For the electron + muon energy resolution, I don't have any real good way -# to estimate this, so we are conservative and set the error to 10%. PRIORS = [ 1.0, # Atmospheric Neutrino Scale 0.0, # Electron energy scale |