格陵兰射电中微子天文台(RNO-G)

S. Wissel, J. Aguilar, P. Allison, J. Beatty, H. Bernhoff, D. Besson, N. Bingefors, O. Botner, S. Bouma, S. Buitink, K. Carter, M. Cataldo, B. Clark, Z. Curtis-Ginsberg, A. Connolly, P. Dasgupta, S. D. Kockere, K. D. Vries, C. Deaconu, M. DuVernois, C. Glaser, A. Hallgren, S. Hallmann, J. Hanson, B. Hendricks, B. Hokanson-Fasig, C. Hornhuber, K. Hughes, A. Karle, J. Kelley, S. Klein, R. Krebs, R. Lahmann, U. Latif, M. Magnuson, T. Meures, Z. Meyers, K. Mulrey, A. Nelles, A. Novikov, E. Oberla, B. Oeyen, H. Pandya, I. Plaisier, L. Pyras, D. Ryckbosch, O. Scholten, D. Seckel, Daniel Smith, D. Southall, J. Torres, S. Toscano, D. Tosi, D. V. D. Broeck, N. Eijndhoven, A. Vieregg, C. Welling, R. Young, A. Zink, Rno-g
{"title":"格陵兰射电中微子天文台(RNO-G)","authors":"S. Wissel, J. Aguilar, P. Allison, J. Beatty, H. Bernhoff, D. Besson, N. Bingefors, O. Botner, S. Bouma, S. Buitink, K. Carter, M. Cataldo, B. Clark, Z. Curtis-Ginsberg, A. Connolly, P. Dasgupta, S. D. Kockere, K. D. Vries, C. Deaconu, M. DuVernois, C. Glaser, A. Hallgren, S. Hallmann, J. Hanson, B. Hendricks, B. Hokanson-Fasig, C. Hornhuber, K. Hughes, A. Karle, J. Kelley, S. Klein, R. Krebs, R. Lahmann, U. Latif, M. Magnuson, T. Meures, Z. Meyers, K. Mulrey, A. Nelles, A. Novikov, E. Oberla, B. Oeyen, H. Pandya, I. Plaisier, L. Pyras, D. Ryckbosch, O. Scholten, D. Seckel, Daniel Smith, D. Southall, J. Torres, S. Toscano, D. Tosi, D. V. D. Broeck, N. Eijndhoven, A. Vieregg, C. Welling, R. Young, A. Zink, Rno-g","doi":"10.22323/1.395.0001","DOIUrl":null,"url":null,"abstract":"The Radio Neutrino Observatory Greenland (RNO-G) is scheduled for deployment in the summerof 2021. It will target the detection of astrophysical and cosmogenic neutrinos above 10 PeV. With 35 autonomous stations, it will be the largest implementation of a radio neutrino detector to date.The stations combine best-practice instrumentation from all previous radio neutrino arrays, such as a deep phased-array trigger and surface antennas. These proceedings describe the experimentalconsiderations that have driven the design of RNO-G and the current progress in deployment, aswell as discuss the projected sensitivity of the instrument. RNO-G will provide a unique view ofthe Northern Sky and will also inform the design of the radio component of IceCube-Gen2.","PeriodicalId":20473,"journal":{"name":"Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)","volume":"98 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2021-09-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"10","resultStr":"{\"title\":\"The Radio Neutrino Observatory Greenland (RNO-G)\",\"authors\":\"S. Wissel, J. Aguilar, P. Allison, J. Beatty, H. Bernhoff, D. Besson, N. Bingefors, O. Botner, S. Bouma, S. Buitink, K. Carter, M. Cataldo, B. Clark, Z. Curtis-Ginsberg, A. Connolly, P. Dasgupta, S. D. Kockere, K. D. Vries, C. Deaconu, M. DuVernois, C. Glaser, A. Hallgren, S. Hallmann, J. Hanson, B. Hendricks, B. Hokanson-Fasig, C. Hornhuber, K. Hughes, A. Karle, J. Kelley, S. Klein, R. Krebs, R. Lahmann, U. Latif, M. Magnuson, T. Meures, Z. Meyers, K. Mulrey, A. Nelles, A. Novikov, E. Oberla, B. Oeyen, H. Pandya, I. Plaisier, L. Pyras, D. Ryckbosch, O. Scholten, D. Seckel, Daniel Smith, D. Southall, J. Torres, S. Toscano, D. Tosi, D. V. D. Broeck, N. Eijndhoven, A. Vieregg, C. Welling, R. Young, A. Zink, Rno-g\",\"doi\":\"10.22323/1.395.0001\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The Radio Neutrino Observatory Greenland (RNO-G) is scheduled for deployment in the summerof 2021. It will target the detection of astrophysical and cosmogenic neutrinos above 10 PeV. With 35 autonomous stations, it will be the largest implementation of a radio neutrino detector to date.The stations combine best-practice instrumentation from all previous radio neutrino arrays, such as a deep phased-array trigger and surface antennas. These proceedings describe the experimentalconsiderations that have driven the design of RNO-G and the current progress in deployment, aswell as discuss the projected sensitivity of the instrument. RNO-G will provide a unique view ofthe Northern Sky and will also inform the design of the radio component of IceCube-Gen2.\",\"PeriodicalId\":20473,\"journal\":{\"name\":\"Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)\",\"volume\":\"98 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2021-09-16\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"10\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.22323/1.395.0001\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.22323/1.395.0001","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 10

摘要

格陵兰射电中微子天文台(RNO-G)计划于2021年夏天部署。它的目标是探测10 PeV以上的天体物理和宇宙中微子。它拥有35个独立的观测站,将是迄今为止最大的射电中微子探测器。这些观测站结合了以前所有射电中微子阵列的最佳实践仪器,如深相控阵触发器和表面天线。这些程序描述了驱动RNO-G设计的实验考虑因素和部署的当前进展,并讨论了仪器的预计灵敏度。RNO-G将提供一个独特的北方天空视图,也将为冰立方- gen2的无线电组件的设计提供信息。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
查看原文
分享 分享
微信好友 朋友圈 QQ好友 复制链接
本刊更多论文
The Radio Neutrino Observatory Greenland (RNO-G)
The Radio Neutrino Observatory Greenland (RNO-G) is scheduled for deployment in the summerof 2021. It will target the detection of astrophysical and cosmogenic neutrinos above 10 PeV. With 35 autonomous stations, it will be the largest implementation of a radio neutrino detector to date.The stations combine best-practice instrumentation from all previous radio neutrino arrays, such as a deep phased-array trigger and surface antennas. These proceedings describe the experimentalconsiderations that have driven the design of RNO-G and the current progress in deployment, aswell as discuss the projected sensitivity of the instrument. RNO-G will provide a unique view ofthe Northern Sky and will also inform the design of the radio component of IceCube-Gen2.
求助全文
通过发布文献求助,成功后即可免费获取论文全文。 去求助
来源期刊
自引率
0.00%
发文量
0
期刊最新文献
The Southern Wide-field Gamma-ray Observatory reach for Primordial Black Hole evaporation Periodicities Observed in Neutron Monitor Counting Rates Throughout Solar Cycles 20-24 Time calibration of the LHAASO-WCDA detectors Energetic particle observations close to the Sun by Solar Orbiter and Parker Solar Probe Nearly a Decade of Cosmic Ray Observations in the Very Local Interstellar Medium
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
现在去查看 取消
×
提示
确定
0
微信
客服QQ
Book学术公众号 扫码关注我们
反馈
×
意见反馈
请填写您的意见或建议
请填写您的手机或邮箱
已复制链接
已复制链接
快去分享给好友吧!
我知道了
×
扫码分享
扫码分享
Book学术官方微信
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术
文献互助 智能选刊 最新文献 互助须知 联系我们:info@booksci.cn
Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。
Copyright © 2023 Book学术 All rights reserved.
ghs 京公网安备 11010802042870号 京ICP备2023020795号-1