P. Allison, J. Beatty, D. Besson, A. Connolly, A. Cummings, C. Deaconu, S. De Kockere, K. D. de Vries, D. Frikken, C. Hast, E. Huesca Santiago, C. -Y. Kuo, A. Kyriacou, U. A. Latif, J. Loonen, I. Loudon, V. Lukic, C. McLennan, K. Mulrey, J. Nam, K. Nivedita, A. Nozdrina, E. Oberla, S. Prohira, J. P. Ralston, M. F. H. Seikh, R. S. Stanley, S. Toscano, D. Van den Broeck, N. van Eijndhoven, S. Wissel
{"title":"宇宙射线雷达回波望远镜（RET-CR）的初步性能","authors":"P. Allison, J. Beatty, D. Besson, A. Connolly, A. Cummings, C. Deaconu, S. De Kockere, K. D. de Vries, D. Frikken, C. Hast, E. Huesca Santiago, C. -Y. Kuo, A. Kyriacou, U. A. Latif, J. Loonen, I. Loudon, V. Lukic, C. McLennan, K. Mulrey, J. Nam, K. Nivedita, A. Nozdrina, E. Oberla, S. Prohira, J. P. Ralston, M. F. H. Seikh, R. S. Stanley, S. Toscano, D. Van den Broeck, N. van Eijndhoven, S. Wissel","doi":"arxiv-2409.07511","DOIUrl":null,"url":null,"abstract":"The Radar Echo Telescope for Cosmic Rays (RET-CR), a pathfinder instrument\nfor the radar echo method of ultrahigh energy (UHE) neutrino detection, was\ninitially deployed near Summit Station, Greenland, in May 2023. After a 4 week\ncommissioning period, 9 days of data were taken before the instrument went\noffline. In this article, we describe the instrument as it was deployed, and\nthe initial performance of the detector. We show that the technical aspects of\nrunning a radar based particle cascade detector in the ice have been\ndemonstrated. Analysis of the 2023 data informed improvements that were\nincorporated into the May-August 2024 deployment, which has just concluded at\ntime of writing. Results from the 2024 run will be presented in forthcoming\npublications.","PeriodicalId":501181,"journal":{"name":"arXiv - PHYS - High Energy Physics - Experiment","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2024-09-11","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Initial performance of the Radar Echo Telescope for Cosmic Rays, RET-CR\",\"authors\":\"P. Allison, J. Beatty, D. Besson, A. Connolly, A. Cummings, C. Deaconu, S. De Kockere, K. D. de Vries, D. Frikken, C. Hast, E. Huesca Santiago, C. -Y. Kuo, A. Kyriacou, U. A. Latif, J. Loonen, I. Loudon, V. Lukic, C. McLennan, K. Mulrey, J. Nam, K. Nivedita, A. Nozdrina, E. Oberla, S. Prohira, J. P. Ralston, M. F. H. Seikh, R. S. Stanley, S. Toscano, D. Van den Broeck, N. van Eijndhoven, S. Wissel\",\"doi\":\"arxiv-2409.07511\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The Radar Echo Telescope for Cosmic Rays (RET-CR), a pathfinder instrument\\nfor the radar echo method of ultrahigh energy (UHE) neutrino detection, was\\ninitially deployed near Summit Station, Greenland, in May 2023. After a 4 week\\ncommissioning period, 9 days of data were taken before the instrument went\\noffline. In this article, we describe the instrument as it was deployed, and\\nthe initial performance of the detector. We show that the technical aspects of\\nrunning a radar based particle cascade detector in the ice have been\\ndemonstrated. Analysis of the 2023 data informed improvements that were\\nincorporated into the May-August 2024 deployment, which has just concluded at\\ntime of writing. Results from the 2024 run will be presented in forthcoming\\npublications.\",\"PeriodicalId\":501181,\"journal\":{\"name\":\"arXiv - PHYS - High Energy Physics - Experiment\",\"volume\":null,\"pages\":null},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-09-11\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - High Energy Physics - Experiment\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2409.07511\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - High Energy Physics - Experiment","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.07511","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Initial performance of the Radar Echo Telescope for Cosmic Rays, RET-CR
The Radar Echo Telescope for Cosmic Rays (RET-CR), a pathfinder instrument
for the radar echo method of ultrahigh energy (UHE) neutrino detection, was
initially deployed near Summit Station, Greenland, in May 2023. After a 4 week
commissioning period, 9 days of data were taken before the instrument went
offline. In this article, we describe the instrument as it was deployed, and
the initial performance of the detector. We show that the technical aspects of
running a radar based particle cascade detector in the ice have been
demonstrated. Analysis of the 2023 data informed improvements that were
incorporated into the May-August 2024 deployment, which has just concluded at
time of writing. Results from the 2024 run will be presented in forthcoming
publications.
京公网安备 11010802042870号
京ICP备2023020795号-1
分享
求助内容：
应助结果提醒方式：
扫码关注我们
