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Ilya Mandel

Researcher at Monash University

Publications -  425
Citations -  55243

Ilya Mandel is an academic researcher from Monash University. The author has contributed to research in topics: Gravitational wave & LIGO. The author has an hindex of 90, co-authored 401 publications receiving 46592 citations. Previous affiliations of Ilya Mandel include Swinburne University of Technology & University of Birmingham.

Papers
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Astrophysical science metrics for next-generation gravitational-wave detectors

TL;DR: In this paper, a set of astrophysically motivated metrics to evaluate the performance of the third-generation laser interferometers in existing km-scale facilities were proposed. And the impact of detector design choices against these metrics, providing a quantitative cost-benefit analyses of the resulting scientific payoffs.
Journal ArticleDOI

Panning for gold, but finding helium: Discovery of the ultra-stripped supernova SN2019wxt from gravitational-wave follow-up observations

TL;DR: In this article , the authors presented the results from multi-wavelength observations of a transient discovered during the follow-up of S191213g, a gravitational wave (GW) event reported by the LIGO-Virgo Collaboration as a possible binary neutron star merger in a low latency search.
Peer Review

Black holes as the end state of stellar evolution: Theory and simulations

TL;DR: In this paper , the authors provide a concise overview of the evolutionary channels that may lead to black hole formation, including the classical route of iron core collapse, collapse due to pair instability in very massive stars, and the hypothetical scenario of supermassive star collapse.

Probing cosmic history with merging compact binaries

Jeff Riley, +1 more
TL;DR: In this article , binary black hole populations are used to measure cosmological parameters describing the redshift-dependent star formation rate and metallicity distribution, and a method that uses artificial neural networks to emulate binary population synthesis computer models is presented.
Journal ArticleDOI

On the maximum stellar rotation to form a black hole without an accompanying luminous transient

TL;DR: In this article, the authors studied the conditions under which infalling material can accrete without forming a centrifugally supported structure and, as a result, generate no effective feedback, and suggested that the event is likely to be followed by a bright transient.