activity
20242026
most citedDecoding Long-duration Gravitational Waves from Binary Neutron Stars with Machine Learning: Parameter Estimation and Equations of State

11 citations · 34 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2026

A NICER view of PSR J16142230: a massive and compact millisecond pulsar

Lucien Mauviard, Sebastien Guillot, Lami Suleiman +17

Using pulse profile modeling, we obtain the mass-radius measurement of a millisecond pulsar (MSP) with data from the Neutron Star Interior Composition ExploreR, XMM-Newton and the…

astro-ph.HE2025

Nuclear parameter inference with semi-agnostic priors

Lami Suleiman, Anthea F. Fantina, Francesca Gulminelli +1

Radio pulsar timing, X-ray pulse profile modeling, and gravitational-wave detections of binary mergers involving at least one neutron star probe the properties of dense, neutron-ri…

astro-ph.HE2025★ 7 cited

Inferring the neutron star equation of state with nuclear-physics informed semiparametric models

Sunny Ng, Isaac Legred, Lami Suleiman +3

Over the past decade, an abundance of information from neutron-star observations, nuclear experiments and theory has transformed our efforts to elucidate the properties of dense ma…

astro-ph.HE2025★ 6 cited

Crust (Unified) Tool for Equation-of-state Reconstruction (CUTER) v2

P. J. Davis, H. Dinh Thi, A. F. Fantina +3

The equation of state (EoS) is a needed input to determine the neutron-star global properties and to relate them. It is thus important to provide consistent and unified EoSs to avo…

gr-qc2024★ 11 cited

Decoding Long-duration Gravitational Waves from Binary Neutron Stars with Machine Learning: Parameter Estimation and Equations of State

Qian Hu, Jessica Irwin, Qi Sun +4

Gravitational waves (GWs) from binary neutron stars (BNSs) offer valuable understanding of the nature of compact objects and hadronic matter, and the science potential will be grea…

astro-ph.HE2024★ 10 cited

Quasi-universal relations in the context of future neutron star detections

Lami Suleiman, Jocelyn Read

The equation of state dependence of neutron star's astrophysical features modeling is key to our understanding of dense matter. However, there exists a series of almost equation-of…