The IceTop Scintillator Upgrade
35th International Cosmic Ray Conference, Bexco, South Korea, 10 Jul 2017 - 20 Jul 2017; Proceedings of Science (ICRC2017), 401 (2017). : The IceCube Neutrino Observatory at the South Pole probes the high-energy cosmic-ray sky byinvestigating the muonic and electromagnetic component of air showers m...
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ftdatacite:10.3204/pubdb-2018-00029 2023-05-15T18:21:53+02:00 The IceTop Scintillator Upgrade Huber, T. Kelley, J. Kunwar, S. Tosi, D. 2017 https://dx.doi.org/10.3204/pubdb-2018-00029 http://bib-pubdb1.desy.de/record/398638 en eng Deutsches Elektronen-Synchrotron, DESY, Hamburg 530 Text Journal article article-journal ScholarlyArticle 2017 ftdatacite https://doi.org/10.3204/pubdb-2018-00029 2021-11-05T12:55:41Z 35th International Cosmic Ray Conference, Bexco, South Korea, 10 Jul 2017 - 20 Jul 2017; Proceedings of Science (ICRC2017), 401 (2017). : The IceCube Neutrino Observatory at the South Pole probes the high-energy cosmic-ray sky byinvestigating the muonic and electromagnetic component of air showers measured with IceTopand the in-ice detector. However, more detailed measurements are needed to understand theastrophysics of the high-energy cosmic-ray sky. This, along with the need to mitigate the impactof snow accumulation on IceTop tanks, has given us impetus for further upgrades includingscintillator and SiPM-readout-based stations.Prototype stations showcasing technologicaladvances for the next generation in cosmic ray detection are currently under construction fordeployment at South Pole in December 2017. We describe the physics and the current status ofthe project. : Published by SISSA, Trieste Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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530 Huber, T. Kelley, J. Kunwar, S. Tosi, D. The IceTop Scintillator Upgrade |
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35th International Cosmic Ray Conference, Bexco, South Korea, 10 Jul 2017 - 20 Jul 2017; Proceedings of Science (ICRC2017), 401 (2017). : The IceCube Neutrino Observatory at the South Pole probes the high-energy cosmic-ray sky byinvestigating the muonic and electromagnetic component of air showers measured with IceTopand the in-ice detector. However, more detailed measurements are needed to understand theastrophysics of the high-energy cosmic-ray sky. This, along with the need to mitigate the impactof snow accumulation on IceTop tanks, has given us impetus for further upgrades includingscintillator and SiPM-readout-based stations.Prototype stations showcasing technologicaladvances for the next generation in cosmic ray detection are currently under construction fordeployment at South Pole in December 2017. We describe the physics and the current status ofthe project. : Published by SISSA, Trieste |
format |
Text |
author |
Huber, T. Kelley, J. Kunwar, S. Tosi, D. |
author_facet |
Huber, T. Kelley, J. Kunwar, S. Tosi, D. |
author_sort |
Huber, T. |
title |
The IceTop Scintillator Upgrade |
title_short |
The IceTop Scintillator Upgrade |
title_full |
The IceTop Scintillator Upgrade |
title_fullStr |
The IceTop Scintillator Upgrade |
title_full_unstemmed |
The IceTop Scintillator Upgrade |
title_sort |
icetop scintillator upgrade |
publisher |
Deutsches Elektronen-Synchrotron, DESY, Hamburg |
publishDate |
2017 |
url |
https://dx.doi.org/10.3204/pubdb-2018-00029 http://bib-pubdb1.desy.de/record/398638 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_doi |
https://doi.org/10.3204/pubdb-2018-00029 |
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1766201223120158720 |