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Eloise M. Biggs

Researcher at University of Western Australia

Publications -  44
Citations -  3877

Eloise M. Biggs is an academic researcher from University of Western Australia. The author has contributed to research in topics: Sustainability & LIGO. The author has an hindex of 22, co-authored 43 publications receiving 2935 citations. Previous affiliations of Eloise M. Biggs include University of Southampton.

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GW190814: Gravitational Waves from the Coalescence of a 23 M$_\odot$ Black Hole with a 2.6 M$_\odot$ Compact Object

R. Abbott, +1254 more
TL;DR: In this article, the authors reported the observation of a compact binary coalescence involving a 22.2 -24.3 magnitude black hole and a compact object with a mass of 2.50 -2.67 magnitude.
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GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4 M_{\odot}$

B. P. Abbott, +1199 more
TL;DR: In 2019, the LIGO Livingston detector observed a compact binary coalescence with signal-to-noise ratio 12.9 as mentioned in this paper, which is consistent with the individual binary components being neutron stars.
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Sustainable development and the water–energy–food nexus: A perspective on livelihoods

TL;DR: In this article, the authors present a critical review of water-energy-food nexus approaches and identify potential linkages with sustainable livelihoods theory and practice, to deepen our understanding of the interrelated dynamics between human populations and the natural environment.
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Properties and astrophysical implications of the 150 Msun binary black hole merger GW190521.

R. Abbott, +1254 more
TL;DR: The GW190521 signal as mentioned in this paper is consistent with a binary black hole merger source at redshift 0.8 with unusually high component masses, and shows mild evidence for spin-induced orbital precession.
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Model comparison from LIGO-Virgo data on GW170817's binary components and consequences for the merger remnant

B. P. Abbott, +1191 more
TL;DR: In this paper, the authors perform Bayesian model selection on a wide range of theoretical predictions for the neutron star equation of state, and find that all scenarios from prompt collapse to long-lived or even stable remnants are possible.