14–24 Jul 2025
CICG - International Conference Centre - Geneva, Switzerland
Europe/Zurich timezone
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Gamma-ray identification with Sb

Not scheduled
20m
Level -1 & 0

Level -1 & 0

Poster Gamma-Ray Astrophysics PO-2

Speaker

Dr Analisa Mariazzi (Instituto de Fisica La Plata)

Description

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.

Collaboration(s) SWGO collaboration

Authors

Dr Patricia Hansen (Instituto de Fisica La Plata) Dr Indira Vergarta Quispe (Instituto de Fisica La Plata) Dr Analisa Mariazzi (Instituto de Fisica La Plata) Prof. Lukas Nellen (nstituto de Ciencias Nucleares, UNAM) Dr Diego Melo (ITeDA)

Presentation materials

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