Volume 501 - 39th International Cosmic Ray Conference (ICRC2025) - Gamma-Ray Astrophysics
Gamma-ray identification with Sb
A.G. Mariazzi*, P.M. Hansen, D. Melo, L. Nellen, I.D. Vergara Quispe  on behalf of the SWGO collaboration
*: corresponding author
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Pre-published on: September 24, 2025
Published on:
Abstract
Gamma-ray observatories must efficiently distinguish gamma-ray-induced showers from the abundant background of hadronic showers. The shape of the lateral signal distribution offers crucial information for this task. Sb is a key observable that characterizes the shape of the lateral signal distribution. It is computed using the signal and position of each triggered detector, along with a free parameter, b. This work investigates the potential of Sb as a robust discriminator for gamma-ray identification in triangular grid arrays with varying detector densities. The behavior of the free parameter b was studied as a function of both the zenith angle and the shower size. A parametrization of b is provided for use in Sb on an event-by-event basis. This parametrization yields improvements in both merit and quality factors for gamma / hadron discrimination, demonstrating that Sb is a powerful separator for next-generation ground-based gamma-ray observatories such as SWGO.
DOI: https://doi.org/10.22323/1.501.0748
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