aboutsummaryrefslogtreecommitdiff
diff options
context:
space:
mode:
authortlatorre <tlatorre@uchicago.edu>2020-12-09 14:16:34 -0600
committertlatorre <tlatorre@uchicago.edu>2020-12-09 14:16:34 -0600
commit5e63a701a8b144093528c063856d513be92a37ed (patch)
tree0d14b914cd8c0f824a9e85159a482e6c0880c991
parentf43a75955e8a624b1927b3075776574303158634 (diff)
downloadsddm-5e63a701a8b144093528c063856d513be92a37ed.tar.gz
sddm-5e63a701a8b144093528c063856d513be92a37ed.tar.bz2
sddm-5e63a701a8b144093528c063856d513be92a37ed.zip
update discovery threshold again
-rwxr-xr-xutils/dm-search2
1 files changed, 1 insertions, 1 deletions
diff --git a/utils/dm-search b/utils/dm-search
index aaac58c..214ad59 100755
--- a/utils/dm-search
+++ b/utils/dm-search
@@ -509,7 +509,7 @@ def get_limits(dm_masses,data,muon,data_mc,atmo_scale_factor,muon_scale_factor,b
# increase our discovery threshold to account for the look
# elsewhere effect.
threshold = DISCOVERY_P_VALUE/(len(bins)-1)
- discovery = max(poisson.ppf(1-threshold,n) - n,0)
+ discovery = poisson.ppf(1-threshold,n) + 1 - n
# Here, we scale the discovery threshold by the fraction of the
# dark matter hist in the histogram range. The idea is that if only
# a small fraction of the dark matter histogram falls into the