报告内容
摘 要
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Advanced LIGO opened an exciting new era for gravitational wave, and consequently for multi-messenger astronomy.
The merger of compact binaries consist neutron stars and/or black holes are anticipated to emit radiation throughout
a wide range of electro-magnetic spectrum (GRB, kilonovae, FRB ...) at very different time scales. An proof-of-principle
method was proposed to optimise the allocation of observation time in order to maximise the detection probability for
kilonovae, while the same idea could be performed on other sources.
A joint detection with multiple messengers can not only provide profound evidence for the physical mechanism for
mysterious phenomenon like GRBs and FRB, but also provide an excellent opportunity to perform a comprehensive
study of the central engine. The concept of an interactive platform to submit observations and getting feedback will
be discussed.
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