The Astrophysical Multimessenger Observatory Network (AMON)

被引:88
作者
Smith, M. W. E. [1 ,2 ]
Fox, D. B. [2 ,3 ]
Cowen, D. F. [1 ,2 ,3 ]
Meszaros, P. [1 ,2 ,3 ]
Tesic, G. [1 ,2 ]
Fixelle, J. [3 ]
Bartos, I. [4 ,5 ]
Sommers, P. [1 ,2 ,3 ]
Ashtekar, Abhay [1 ,2 ]
Babu, G. Jogesh [3 ,6 ]
Barthelmy, S. D. [7 ]
Coutu, S. [1 ,2 ]
DeYoung, T. [1 ,2 ]
Falcone, A. D. [2 ,3 ]
Gao, Shan [1 ,2 ]
Hashemi, B. [1 ]
Homeier, A. [8 ]
Marka, S. [4 ,5 ]
Owen, B. J. [1 ,2 ]
Taboada, I. [9 ]
机构
[1] Penn State Univ, Dept Phys, University Pk, PA 16802 USA
[2] Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA
[3] Penn State Univ, Dept Astron & Astrophys, University Pk, PA 16802 USA
[4] Columbia Univ, Dept Phys, New York, NY 10027 USA
[5] Columbia Univ, Columbia Astrophys Lab, New York, NY 10027 USA
[6] Penn State Univ, Dept Stat, University Pk, PA 16802 USA
[7] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[8] Univ Bonn, Inst Phys, D-53115 Bonn, Germany
[9] Georgia Inst Technol, Sch Phys, Ctr Relativist Astrophys, Atlanta, GA 30332 USA
基金
美国国家科学基金会;
关键词
High-energy astrophysics; Gravitational radiation; Neutrinos; Cosmic rays; Gamma-ray bursts; Supernovae; GAMMA-RAY BURSTS; HIGH-ENERGY NEUTRINOS; LARGE-AREA TELESCOPE; GRAVITATIONAL-WAVE BURSTS; PRIMORDIAL BLACK-HOLES; GLUON-JET EMISSION; COSMIC-RAYS; RELATIVISTIC JETS; QUARK-JET; SUPERNOVA;
D O I
10.1016/j.astropartphys.2013.03.003
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We summarize the science opportunity, design elements, current and projected partner observatories, and anticipated science returns of the Astrophysical Multimessenger Observatory Network (AMON). AMON will link multiple current and future high-energy, multimessenger, and follow-up observatories together into a single network, enabling near real-time coincidence searches for multimessenger astrophysical transients and their electromagnetic counterparts. Candidate and high-confidence multimessenger transient events will be identified, characterized, and distributed as AMON alerts within the network and to interested external observers, leading to follow-up observations across the electromagnetic spectrum. In this way, AMON aims to evoke the discovery of multimessenger transients from within observatory subthreshold data streams and facilitate the exploitation of these transients for purposes of astronomy and fundamental physics. As a central hub of global multimessenger science, AMON will also enable cross-collaboration analyses of archival datasets in search of rare or exotic astrophysical phenomena. (C) 2013 Elsevier B.V. All rights reserved.
引用
收藏
页码:56 / 70
页数:15
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