sddm/src/.gitignore, branch master Code for the self-destructing dark matter search in SNO extend electron range tables up to 1 TeV 2020-04-14T17:01:43+00:00 tlatorre tlatorre@uchicago.edu 2020-04-14T17:01:43+00:00 2a5152b03b6d4027b52e625c3b94a436313373be 






add zdab-cat
2019-05-23T15:22:15+00:00

tlatorre
tlatorre@uchicago.edu

2019-05-23T15:22:15+00:00

f332b293430d5641575917686d7dc128c309acf5

This commit adds a new program called zdab-cat which is kind of like fit, but
just produces the YAML output without actually fitting anything.





This commit adds a new program called zdab-cat which is kind of like fit, but
just produces the YAML output without actually fitting anything.







add rayleigh scattering
2018-11-27T22:07:56+00:00

tlatorre
tlatorre@uchicago.edu

2018-11-27T22:07:56+00:00

a0c1f4560325311558eedf39bd191ddaad182367

This commit adds Rayleigh scattering to the likelihood function. The Rayleigh
scattering lengths come from rsp_rayleigh.dat from SNOMAN which only includes
photons which scattered +/- 10 ns around the prompt peak. The fraction of light
which scatters is treated the same in the likelihood as reflected light, i.e.
it is uniform across all the PMTs in the detector and the time PDF is assumed
to be a constant for a fixed amount of time after the prompt peak.





This commit adds Rayleigh scattering to the likelihood function. The Rayleigh
scattering lengths come from rsp_rayleigh.dat from SNOMAN which only includes
photons which scattered +/- 10 ns around the prompt peak. The fraction of light
which scatters is treated the same in the likelihood as reflected light, i.e.
it is uniform across all the PMTs in the detector and the time PDF is assumed
to be a constant for a fixed amount of time after the prompt peak.







update .gitignore
2018-11-26T16:35:58+00:00

tlatorre
tlatorre@uchicago.edu

2018-11-26T16:35:58+00:00

b7a56ddb43d3d3066806722da4d1c812ed1ad028












update electron range tables
2018-11-26T15:53:28+00:00

tlatorre
tlatorre@uchicago.edu

2018-11-26T15:53:28+00:00

9777b92d16cb3a3434c43b084d88f59321567e2d

This commit also adds a script to calculate the CSDA range for electrons from a
table of the stopping power as a function of energy. We need this script since
the NIST ESTAR website will only output the stopping power above a certain
energy threshold (1 GeV for electrons).

See https://physics.nist.gov/PhysRefData/Star/Text/ESTAR.html.





This commit also adds a script to calculate the CSDA range for electrons from a
table of the stopping power as a function of energy. We need this script since
the NIST ESTAR website will only output the stopping power above a certain
energy threshold (1 GeV for electrons).

See https://physics.nist.gov/PhysRefData/Star/Text/ESTAR.html.