The Swift short gamma-ray burst rate density: implications for binary neutron star merger rates
Author:
Affiliation:
1. School of Physics; University of Western Australia; Crawley; WA; 6009; Australia
2. Racah Institute of Physics; The Hebrew University; Jerusalem; 91904; Israel
3. ASI Science Data Center; via Galileo Galilei; 00044; Frascati (RM); Italy
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/425/4/2668/4895856/425-4-2668.pdf
Reference60 articles.
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3. Comparison of the Gamma‐Ray Burst Sensitivity of Different Detectors
4. Postlaunch Analysis ofSwift’s Gamma‐Ray Burst Detection Sensitivity
5. On the Rarity of Double Black Hole Binaries: Consequences for Gravitational Wave Detection
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