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

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>