Eitan Buffaz

ORCID: 0000-0003-2205-2912
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About
Contact & Profiles
Research Areas
  • Pulsars and Gravitational Waves Research
  • Seismology and Earthquake Studies
  • Gamma-ray bursts and supernovae
  • Seismic Waves and Analysis

McGill University
2022-2024

Abstract GWSkyNet-Multi is a machine learning model developed for the classification of candidate gravitational-wave events detected by LIGO and Virgo observatories. The uses limited information released in low-latency Open Public Alerts to produce prediction scores indicating whether an event merger two black holes (BHs), involving neutron star (NS), or non-astrophysical glitch. This facilitates time-sensitive decisions about perform electromagnetic follow-up during LIGO-Virgo-KAGRA (LVK)...

10.3847/1538-4357/ad13ea article EN cc-by The Astrophysical Journal 2024-03-01

Abstract Compact object mergers which produce both detectable gravitational waves and electromagnetic (EM) emission can provide valuable insights into the neutron star equation of state, tension in Hubble constant, origin r -process elements. However, EM follow-up wave sources is complicated by false-positive detections, transient nature associated emission. GWSkyNet-Multi a machine learning model that attempts facilitate providing real-time predictions source detection. The uses information...

10.3847/1538-4357/ac5019 article EN cc-by The Astrophysical Journal 2022-03-01

GWSkyNet-Multi is a machine learning model developed for classification of candidate gravitational-wave events detected by the LIGO and Virgo observatories. The uses limited information released in low-latency Open Public Alerts to produce prediction scores indicating whether an event merger two black holes, involving neutron star, or non-astrophysical glitch. This facilitates time sensitive decisions about perform electromagnetic follow-up during LIGO-Virgo-KAGRA (LVK) observing runs....

10.48550/arxiv.2308.12357 preprint EN cc-by arXiv (Cornell University) 2023-01-01
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