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Physical Review D

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Results from an injection and recovery study involving 35 numerical relativity simulations and three waveform models

Sarp Akçay1, Charlie Hoy2, and Jake Mac Uilliam1,3

Parameter estimation for the GWTC-4.0 catalog with phenomenological waveform models that include orbital eccentricity and an updated description of spin precession

Yumeng Xu, Jorge Valencia, Héctor Estellés Estrella, Antoni Ramos-Buades, Sascha Husa, Maria Rosselló-Sastre, Joan Llobera Querol, Felip A. Ramis Vidal, Maria de Lluc Planas Llompart, Marta Colleoni, Eleanor Hamilton, Arnau Montava Agudo, Jesús Yébana Carrilero, and Anna Heffernan

Phys. Rev. D 113 083001 (2026)

Improved gravitational wave model linking precessing inspirals and numerical-relativity-calibrated merger-ringdown

Eleanor Hamilton, Marta Colleoni, Jonathan E. Thompson, Charlie Hoy, Anna Heffernan, Meryl Kinnear, Jorge Valencia, Felip A. Ramis Vidal, Cecilio García-Quirós, Shrobana Ghosh, Lionel London, Mark Hannam, and Sascha Husa

Phys. Rev. D 113 084055 (2026)

Reconsidering the consistent use of precessing, higher order multipole models for gravitational wave analyses

C Hoy

Monthly Notices of the Royal Astronomical Society 549 stag898 (2026)

The missing multipole problem: investigating biases from model starting frequency in gravitational-wave analyses

R Ursell, C Hoy, I Harry, and L K Nuttall

Monthly Notices of the Royal Astronomical Society 547 stag398 (2026)

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