Abstract
The Southern Wide-field Gamma-ray Observatory (SWGO) will use the well-established and cost-effective technique of detecting Cherenkov light produced in water-filled detection units for TeV gamma-ray astronomy. Leveraging detector material reflectivity together with an optimised aspect ratio is an option to improve the performance of an array of such detector units. The double-layered Water Cherenkov Detector units comprise chambers with single photosensors in each. A reflective upper compartment enhances sensitivity to impinging secondary particles. A shallow lower compartment enables muon tagging and consequently improves the gamma hadron separation power of the observatory. Here we present detailed studies on the double-layered unit design.
Original language | English |
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Title of host publication | Double-layered Water Cherenkov Detector for SWGO |
Volume | 395 |
Publication status | Published - 18 Mar 2022 |
Event | 37th International Cosmic Ray Conference, ICRC 2021 - Virtual, Berlin, Germany Duration: 12 Jul 2021 → 23 Jul 2021 |
Publication series
Name | Proceedings of Science |
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Publisher | Sissa Medialab Srl |
Conference
Conference | 37th International Cosmic Ray Conference, ICRC 2021 |
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Country/Territory | Germany |
City | Virtual, Berlin |
Period | 12/7/21 → 23/7/21 |
Bibliographical note
Publisher Copyright:© Copyright owned by the author(s) under the terms of the Creative Commons.
All Science Journal Classification (ASJC) codes
- General