Multi-messenger study at the Pierre Auger Observatory

来源 :第8届高海拔宇宙线探测国际研讨会(The 8th International Workshop on Air Showe | 被引量 : 0次 | 上传用户:kf3567
下载到本地 , 更方便阅读
声明 : 本文档内容版权归属内容提供方 , 如果您对本文有版权争议 , 可与客服联系进行内容授权或下架
论文部分内容阅读
Taken from Ana Franckowiaks talk Why multimessenger? How? Reveal the existence of hidden sources opaque to hadrons and photons Escaping gravitational wave and neutrinos from Inner region
其他文献
OUTLINE Background NG-DRAPS Future Plan New technology→Data Rate VLBI High stability frequency standard High accuracy time synchronization High speed recording
会议
Outline Background of LSI+61 303 VLBA Observations Results Future Plan Background of LSI+61 303Binary:Be star(B0)+compact object Microquasar or Pulsar wind D~2 k
会议
Outline Broadband Cryogenic Receiver(1.2-6.9 GHz)Feed & LNA Research Broadband Receivers Review
会议
Outline VLBI system of FAST Introduction Test of Roach2 & Mark IV Plan of test observation Drift mode Tracking mode
会议
分析了UT1实验及初步结果,介绍了DiFX+AIPS数据检查、比较了几何时延模型、进行了时频稳定性评估实验。初步走通UT1流程,具备天体测量和成图观测能力。
介绍了CEI测量系统结构、分析了测量结果以及CEI技术在GEO卫星轨道监测中的应用。增加实时标校后,改善了观测的数据质量;尤其对于白天的数据;气温变化引起电缆温度变化对观测相
LHAASO could provide useful data on solar diurnal anisotropy~100 GeV LHAASO may reconstruct shower events for cosmic rays down to about~100 GeV.
会议
Summary ·Background and Motivation ·3-D Forbush Decrease Numerical Model · Simulation Results ·Conclusion
会议
24 Medium Size Telescopes 12m diameter Mirror 200 GeV-10 TeV 70 Small Size Telescopes 4m diameter mirror 1 TeV-200 TeV 4 Large Size Telescopes 24m Diameter Mirr
会议
Spectrum of CRs ·Above ‘ankle’:extragalactic ·Below ‘knee’:galactic origin(Gal.E.den.> SMC E.den) Two great ideas in a single short paper
会议