On the likelihood of detecting gravitational waves from Population III compact object binaries-Reference-Cited by-同舟云学术

On the likelihood of detecting gravitational waves from Population III compact object binaries

Author:

Belczynski Krzysztof¹²,Ryu Taeho³,Perna Rosalba³,Berti Emanuele⁴^ORCID,Tanaka Takamitsu L.²,Bulik Tomasz²⁵

Affiliation:

1. Nicolaus Copernicus Astronomical Centre, Polish Academy of Sciences, ul. Bartycka 18, PL-00-716 Warsaw, Poland

2. Astronomical Observatory, Warsaw University, Ujazdowskie 4, PL-00-478 Warsaw, Poland

3. Department of Physics and Astronomy, Stony Brook University, Stony Brook, NY 11794-3800, USA

4. Department of Physics and Astronomy, The University of Mississippi, University, MS 38677, USA

5. Instituto de Astronomía, Universidad Nacional Autónoma de México. Km 103 Carretera Tijuana-Ensenada, 22860 Ensenada, Baja California, Mexico

Funder

NCN

Stony Brook University

NSF

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

Reference100 articles.

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