Exploring the supernova remnant contribution to the first LHAASO source catalog via passively illuminated interstellar clouds

Autor: Mitchell, Alison M.W., Celli, Silvia

Publikováno v: In Journal of High Energy Astrophysics November 2024 44:340-355

Exploring the population of Galactic very-high-energy γ-ray sources

Autor: CTA Consortium, Steppa, Constantin, Egberts, Kathrin, Abdalla, Hassan, Abe, H., Abe, S., Abusleme, Ángel, Acero, Fabio, Acharyya, Atreya, Acín Portella, V., Ackley, Kendall, Adam, R., Adams, Carl B., Adhikari, S. S., Aguado-Ruesga, I., Agudo, Iván, Aguilera, R., Aguirre-Santaella, Alejandra, Aharonian, F., Alberdi A., Alfaro, Rubén, Arbet-Engels, Axel, Biland, Adrian, Mitchell, Alison M.W., Neise, Dominik

Publikováno v: Proceedings of Science, 395:798. Sissa Medialab Srl
PoS: Proceedings of Science, 395
Proceedings of 37th International Cosmic Ray Conference

At very high energies (VHE), the emission of γ rays is dominated by discrete sources. Due to the limited resolution and sensitivity of current-generation instruments, only a small fraction of the total Galactic population of VHE γ-ray sources has b

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2257b652850bc75b76974b20bd829c20
https://dare.uva.nl/personal/pure/en/publications/exploring-the-population-of-galactic-veryhighenergy-ray-sources(ecfda8f4-e8f0-49f1-9020-9b18f2ccaed1).html

Performance of the Cherenkov Telescope Array in the presence of clouds

Autor: Cherenkov Telescope Array Consortium, Pecimotika, Mario, Adamczyk, Katarzyna, Dominis Prester, Dijana, Gueta, Orel, Hrupec, Dario, Maier, Gernot, Mićanović, Saša, Pavletić, Lovro, Sitarek, Julian, Sobczyńska, Dorota, Szanecki, Michał, Abdalla, Hassan, Abe, H., Abe, S., Abusleme, Ángel, Acero, Fabio, Acharyya, Atreya, Acín Portella, V., Ackley, Kendall, Adam, R., Arbet-Engels, Axel, Biland, Adrian, Mitchell, Alison M.W., Neise, Dominik

Publikováno v: PoS: Proceedings of Science, 395
Proceedings of 37th International Cosmic Ray Conference

The Cherenkov Telescope Array (CTA) is the future ground-based observatory for gamma-ray astronomy at very high energies. The atmosphere is an integral part of every Cherenkov telescope. Different atmospheric conditions, such as clouds, can reduce th

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ab4bf9473613ca1abb95aaba5dea0073

Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

Autor: CTA Consortium, Abdalla, Hassan, Abe, H., Abe, S., Abusleme, Ángel, Acero, Fabio, Acharyya, Atreya, Acín Portella, V., Ackley, Kendall, Adam, R., Adams, Carl B., Adhikari, S. S., Aguado-Ruesga, I., Agudo, Ivan, Aguilera, R., Aguirre-Santaella, Alejandra, Aharonian, F., Alberdi A., Alfaro, Rubén, Alfaro, Jorge, Alispach, Cyril, Arbet Engels, A., Biland, Adrian, Mitchell, Alison M.W., Neise, Dominik

Publikováno v: PoS: Proceedings of Science, 395
Proceedings of 37th International Cosmic Ray Conference

High-energy gamma rays are promising tools to constrain or reveal the nature of dark matter, in particular Weakly Interacting Massive Particles. Being well into its pre-construction phase, the Cherenkov Telescope Array (CTA) will soon probe the sky i

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4a9cdff6ea36c4cf83611e9f424b9b27

Searching for Dark Matter with the Southern Wide-field Gamma-ray Observatory (SWGO)

Autor: SWGO Collaboration, Viana, Aion, Albert, Andrea, Harding, J. Patrick, Hinton, Jim A., Schoorlemmer, Harm, De Souza, Vitor, Abreu, Pedro, Angüner, E. O., Arcaro, Cornelia H.E., Arnaldi, L. H., Arteaga-Velàzquez, Juan Carlos, Assis, Pedro, Bakalová, A., Barres de Almeida, Ulisses, Batković, Ivana, Bellido, J. A., Belmont-Moreno, Ernesto, Bisconti, Francesca, Blanco, A., Mitchell, Alison M.W.

Publikováno v: PoS: Proceedings of Science, 395
Proceedings of 37th International Cosmic Ray Conference

Despite mounting evidence that dark matter (DM) exists in the Universe, its fundamental nature remains unknown. We present sensitivity estimates to detect DM particles with a future very-high-energy (& TeV) wide field-of-view gamma-ray observatory in

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4247c955006d3b8a53ef82fa7fff7a54