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About
Contact & Profiles
Research Areas
- Pulsars and Gravitational Waves Research
- Magnetic confinement fusion research
- Geophysics and Gravity Measurements
- Astrophysical Phenomena and Observations
- High-pressure geophysics and materials
Northwestern University
2020
I. M. Romero-Shaw
C. Talbot
S. Biscoveanu
V. D’Emilio
G. Ashton
and 54
more
C. P. L. Berry
Scott Coughlin
S. Galaudage
C. G. Hoy
M. T. Hübner
K. S. Phukon
M. Pitkin
Monica Rizzo
Nikhil Sarin
R. J. E. Smith
S. P. Stevenson
A. Vajpeyi
M. Arène
K Athar
S. Banagiri
N. Bose
M. F. Carney
Katerina Chatziioannou
J. A. Clark
M. Colleoni
R. Cotesta
B. Edelman
H. Estellés
C. García-Quirós
Abhirup Ghosh
R. Green
C-J Haster
S. Husa
D. Keitel
A X Kim
F Vivanco
I. Magaña Hernandez
Christos Karathanasis
P. D. Lasky
N. De Lillo
M. E. Lower
D. M. Macleod
M. Mateu-Lucena
A. L. Miller
M. Millhouse
S. Morisaki
S. H. Oh
Serguei Ossokine
Ethan Payne
J. Powell
G. Pratten
M. Pürrer
A. Ramos-Buades
V. Raymond
E. Thrane
J. Veitch
D. R. Williams
M. J. Williams
S. Xiao
ABSTRACT Gravitational waves provide a unique tool for observational astronomy. While the first LIGO–Virgo catalogue of gravitational-wave transients (GWTC-1) contains 11 signals from black hole and neutron star binaries, number observations is increasing rapidly as detector sensitivity improves. To extract information observed signals, it imperative to have fast, flexible, scalable inference techniques. In previous paper, we introduced bilby: modular user-friendly Bayesian library adapted...
10.1093/mnras/staa2850
article
EN
Monthly Notices of the Royal Astronomical Society
2020-09-18
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