Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Mitchell, Alison M. W."'
Publikováno v:
2024 Res. Notes AAS 8 91
This research note concerns the application of deep-learning-based multi-view-imaging techniques to data from the H.E.S.S. Imaging Atmospheric Cherenkov Telescope array. We find that the earlier the fusion of layer information from different views ta
Externí odkaz:
http://arxiv.org/abs/2403.18516
Autor:
Mitchell, Alison M. W., Morlino, Giovanni, Celli, Silvia, Menchiari, Stefano, Specovius, Andreas
Young & massive stellar clusters (SCs) are a potential source of galactic cosmic rays up to very high energies as a result of two possible acceleration scenarios. Collective stellar winds from massive member stars form a wind-blown bubble with a term
Externí odkaz:
http://arxiv.org/abs/2403.16650
Publikováno v:
PoS(ICRC2023)690
Recent results from LHAASO and Tibet AS$\gamma$ suggest that the Crab Nebula's gamma-ray spectrum extends to the PeV energy range, however the production mechanisms of this highest energy emission remain unclear. It has been postulated that a seconda
Externí odkaz:
http://arxiv.org/abs/2310.07429
Publikováno v:
Proceedings of the 38th International Cosmic Ray Conference (ICRC2023). PoS(ICRC2023)694
The number of satellites launched into low earth orbit has almost tripled (to over 4000) in the last three years due to the increasing commercialisation of space. Satellite constellations with a total of over 400,000 satellites are proposed to be lau
Externí odkaz:
http://arxiv.org/abs/2308.01509
Publikováno v:
A&A 677, A141 (2023)
The number of satellites launched into Earth's orbit has almost tripled in the last three years due to the increasing commercialisation of space. Multiple satellite constellations, consisting of over 400,000 individual satellites, have either been pa
Externí odkaz:
http://arxiv.org/abs/2307.13293
Galaxy evolution is an important topic, and our physical understanding must be complete to establish a correct picture. This includes a thorough treatment of feedback. The effects of thermal-mechanical and radiative feedback have been widely consider
Externí odkaz:
http://arxiv.org/abs/2306.09924
In what will likely be a litany of generative-model-themed arXiv submissions celebrating April the 1st, we evaluate the capacity of state-of-the-art transformer models to create a paper detailing the detection of a Pulsar Wind Nebula with a non-exist
Externí odkaz:
http://arxiv.org/abs/2303.17853
Publikováno v:
Eur. Phys. J. C 82, 1118 (2022)
Identification of Cherenkov light generated by muons has been suggested as a promising way to dramatically improve the background rejection power of Imaging Atmospheric Cherenkov Telescope (IACT) arrays at high energies. However, muon identification
Externí odkaz:
http://arxiv.org/abs/2211.13167
The presence of muons in air-showers initiated by cosmic ray protons and nuclei is well established as a powerful tool to separate such showers from those initiated by gamma rays. However, so far this approach has been fully exploited only for ground
Externí odkaz:
http://arxiv.org/abs/2111.12041
Autor:
Baumgartner, Sandra, Bernardini, Mauro, Cuissa, José R. Canivete, de Laroussilhe, Hugues, Mitchell, Alison M. W., Neuenschwander, Benno A., Saha, Prasenjit, Schaeffer, Timothée, Soyuer, Deniz, Zwick, Lorenz
Compact Galactic binary systems with orbital periods of a few hours are expected to be detected in gravitational waves (GW) by LISA or a similar mission. At present, these so-called verification binaries provide predictions for GW frequency and ampli
Externí odkaz:
http://arxiv.org/abs/2008.11538