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Expected performanc...
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Bianciotto, MartaUniversità degli studi di Torino, Via Pietro Giuria 1 10125, Torino, Italy, Via Pietro Giuria 1
(författare)
Expected performance of the K-EUSO space-based observatory
- Artikel/kapitelEngelska2022
Förlag, utgivningsår, omfång ...
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Sissa Medialab Srl,2022
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LIBRIS-ID:oai:DiVA.org:kth-333525
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https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-333525URI
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Språk:engelska
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Sammanfattning på:engelska
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Ämneskategori:ref swepub-contenttype
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Ämneskategori:kon swepub-publicationtype
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QC 20230802
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K-EUSO is a planned mission of the JEM-EUSO program for the study of ultra-high energy cosmic rays (UHECR) from space, to be deployed on the International Space Station. The K-EUSO observatory consists of a UV telescope with a wide field of view, which aims at the detection of fluorescence light emitted by extensive air showers (EAS) in the atmosphere. The EAS events will be sampled with a time resolution of 1-2.5 μs to reconstruct the entire shower profile with high precision. The detector consisting of ∼ 105 independent pixels will allow a spatial resolution of ∼700 m on ground. From a 400 km altitude, K-EUSO will achieve a large and full sky exposure to sample the highest energy range of the UHECR spectrum. In this contribution, we present estimates of the performance of the observatory: an estimation of the expected exposure and triggered event rate as a function of energy and the event reconstruction performance, including resolution of arrival directions and energy of UHECRs.
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Bolmgren, KarlKTH,Partikel- och astropartikelfysik(Swepub:kth)u1la6up4
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Carlson, PerKTH,Partikel- och astropartikelfysik(Swepub:kth)u1ua4u32
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Fuglesang, Christer,1957-KTH,Partikel- och astropartikelfysik(Swepub:kth)u14h36o6
(författare)
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Zuccaro Marchi, A.RIKEN, Wako, Saitama, Japan, Saitama
(författare)
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Università degli studi di Torino, Via Pietro Giuria 1 10125, Torino, Italy, Via Pietro Giuria 1Partikel- och astropartikelfysik
(creator_code:org_t)
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Ingår i:37th International Cosmic Ray Conference, ICRC 2021: Sissa Medialab Srl
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