Kilonova Emission from Black Hole–Neutron Star Mergers. II. Luminosity Function and Implications for Target-of-opportunity Observations of Gravitational-wave Triggers and Blind Searches-Reference-Cited by-同舟云学术

Kilonova Emission from Black Hole–Neutron Star Mergers. II. Luminosity Function and Implications for Target-of-opportunity Observations of Gravitational-wave Triggers and Blind Searches

Published:2021-08-01 Issue:1 Volume:917 Page:24
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Zhu Jin-Ping^ORCID,Wu Shichao^ORCID,Yang Yuan-Pei^ORCID,Zhang Bing^ORCID,Gao He^ORCID,Yu Yun-Wei^ORCID,Li Zhuo,Cao Zhoujian^ORCID,Liu Liang-Duan^ORCID,Huang Yan,Zhang Xing-Han

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/abfe5e/pdf

Reference288 articles.

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4. Properties of the Binary Neutron Star Merger GW170817

5. GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

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