author={R. Ballabriga and J. Braach and E. Buschmann and M. Campbell and D. Dannheim and K. Dort and L. Huth and I. Kremastiotis and J. Kröger and L. Linssen and M. Munker and P. Schütze and W. Snoeys and S. Spannagel and T. Vanat},
}
@software{garfieldpp,
author={{Heinrich Schindler}},
title={Garfield++},
url={https://gitlab.cern.ch/garfield/garfieldpp},
}
@article{rd50ionization,
title={Study of impact ionization coefficients in silicon with Low Gain Avalanche Diodes},
@@ -52,6 +52,7 @@ This geometry can be selected using `geometry = hexagon`
## Radial Strips
Radial strip detectors feature a trapezoidal shape with curved edges and radial geometry – the strips on such a sensor are arranged in a fan-like geometry, pointing to a common focal point. Shape, size and segmentation of a radial strip detector are defined using four parameters, each passed as an array with the number of elements equal to the number of strip rows:
@@ -58,6 +58,7 @@ Note: Neutrons have a lifetime of 882 seconds and will not be propagated in the
*`output_plots_scale` : Set the x-axis scale of the output plot, defaults to 100ke.
### CRY Framework Parameters
*`latitude`: Latitude for which the incident particles from cosmic ray showers should be simulated. Should be between `90.0` (north pole) and `-90.0` (south pole). Defaults to `53.0` (DESY).
*`date`: Date for the simulation to account for the 11-year cycle of solar activity and related change in cosmic ray flux. Should be given as string in the form `month-day-year` and defaults to the last day of 2020, i.e. `12-31-2020`.
*`return_neutrons`: Boolean to select whether neutrons should be returned to Geant4. Defaults to `true`.