Skip to content
This repository has been archived by the owner on Aug 10, 2021. It is now read-only.

Estimate the ACP Integral Spectral Exclusion Zone to calculate time-to-detections in the gamma-ray sky.

License

Notifications You must be signed in to change notification settings

cherenkov-plenoscope/instrument_sensitivity_function

Repository files navigation

ARCHIVE

This repository is out of service. Thanks to Max L. Ahnen for his work. Parts of repositorry life on in starter_kit/plenoirf.

Instrument Sensitivity Function

License: GPL v3 Arxiv DOI

for the Atmospheric Cherenkov Plenoscope (ACP)

Takes the Instrument Response Functions (IRF)s of an ACP to estimate the time-to-detections for known sources in the gamma-ray sky.

installation

git clone https://github.com/TheBigLebowSky/instrument_sensitivity_function.git
cd instrument_sensitivity_function/
pip install -r requirements.txt

Usage Estimate the Integral Spectral Exclusion Zone (ISEZ)

acp_isez --in=<in folder to where the csvs are>  --cutoff=10e-3 # 10GV --rel_flux=0.05<rel. flux secondary to primary particles> --fov=6.5 <in degree> --src=<3FGL name of comparison source> --out=<folder>

About

Estimate the ACP Integral Spectral Exclusion Zone to calculate time-to-detections in the gamma-ray sky.

Resources

License

Stars

Watchers

Forks

Releases

No releases published

Packages

No packages published

Languages