期刊
ASTROPHYSICAL JOURNAL LETTERS
卷 891, 期 2, 页码 -出版社
IOP Publishing Ltd
DOI: 10.3847/2041-8213/ab77c9
关键词
Astrophysical black holes; Gravitational wave astronomy; Astronomy data analysis; Hierarchical models
资金
- NSF Graduate Research Fellowship Program [DGE-1746045]
- NSF [PHY-1708081, PHY-1748958]
- Kavli Institute for Cosmological Physics at the University of Chicago through NSF [PHY-1125897]
- Kavli Foundation
- Marion and Stuart Rice Award
- Simons Foundation
- U.S. National Science Foundation
- French Centre National de Recherche Scientifique (CNRS)
- Italian Istituto Nazionale della Fisica Nucleare (INFN)
- Dutch Nikhef
- Polish institute
- Hungarian institute
Advanced LIGO and Virgo detected 10 binary black holes (BBHs) in their first two observing runs (O1 and O2). Analysis of these events found evidence for a dearth of BBHs with component masses greater than similar to 45 M 45 M at M, it would be common for the most massive system to have an observed maximum-likelihood mass m(1) greater than or similar to 70 M.
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