Distinguishing double neutron star from neutron star-black hole binary populations with gravitational wave observations-Reference-Cited by-同舟云学术

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Distinguishing double neutron star from neutron star-black hole binary populations with gravitational wave observations

Published:2020-07-20 Issue:2 Volume:102 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Fasano Margherita,Wong Kaze W. K.^ORCID,Maselli Andrea^ORCID,Berti Emanuele^ORCID,Ferrari Valeria,Sathyaprakash B. S.^ORCID

Funder

National Science Foundation

National Aeronautics and Space Administration

European Cooperation in Science and Technology

Ministero dell’Istruzione, dell’Università e della Ricerca

Amaldi Research Center

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.102.023025/fulltext

Reference132 articles.

1. Observation of Gravitational Waves from a Binary Black Hole Merger

2. GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence

3. GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2

4. Erratum: GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2 [Phys. Rev. Lett. 118 , 221101 (2017)]

5. GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence

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