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Galactic Science with the Southern Wide-field Gamma-ray Observatory

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conference contribution
posted on 2025-04-09, 13:58 authored by P Abreu, A Albert, EO Angüner, C Arcaro, LH Arnaldi, JC Arteaga-Velázquez, P Assis, A Bakalová, UB de Almeida, I Batković, J Bellido, E Belmont-Moreno, F Bisconti, A Blanco, M Bohacova, E Bottacini, T Bretz, C Brisbois, P Brogueira, AM Brown, T Bulik, KS Caballero Mora, SM Campos, A Chiavassa, L Chytka, R Conceição, G Consolati, J Cotzomi Paleta, S Dasso, A De Angelis, CR De Bom, E de la Fuente, V de Souza, D Depaoli, G Di Sciascio, CO Dib, D Dorner, M Doro, M Du Vernois, T Ergin, KL Fan, N Fraija, S Funk, JI García, JA García-González, ST García Roca, G Giacinti, H Goksu, BS González, F Guarino, A Guillén, F Haist, PM Hansen, JP Harding, J Hinton, W Hofmann, B Hona, D Hoyos, P Huentemeyer, F Hueyotl-Zahuantitla, A Insolia, P Janecek, V Joshi, B Khelifi, S Kunwar, G La Mura, J Lapington, MR Laspiur, F Leitl, F Longo, L Lopes, R Lopez-Coto, D Mandat, AG Mariazzi, M Mariotti, A Marques Moraes, J Martínez-Castro, H Martínez-Huerta, S May, DG Melo, LF Mendes, LM Mendes, T Mineeva, A Mitchell, S Mohan, OG Morales Olivares, E Moreno-Barbosa, L Nellen, V Novotny, L Olivera-Nieto, E Orlando, M Pech, A Pichel, M Pimenta, MP de Albuquerque, E Prandini, MS Rado Cuchills, A Reisenegger, B Reville, CD Rho
The Southern Wide-field Gamma-ray Observatory (SWGO) is a proposed ground-based gamma-ray detector that will be located in the Southern Hemisphere and is currently in its design phase. In this contribution, we will outline the prospects for Galactic science with this Observatory. Particular focus will be given to the detectability of extended sources, such as gamma-ray halos around pulsars; optimisation of the angular resolution to mitigate source confusion between known TeV sources; and studies of the energy resolution and sensitivity required to study the spectral features of PeVatrons at the highest energies. Such a facility will ideally complement contemporaneous observatories in studies of high energy astrophysical processes in our Galaxy.

History

Author affiliation

School of Physics

Source

37th International Cosmic Ray Conference (ICRC2021)

Version

  • VoR (Version of Record)

Published in

Proceedings of Science

Volume

395

Publisher

Sissa Medialab srl Partita

eissn

1824-8039

Copyright date

2022

Available date

2025-04-09

Language

en

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