works on

From the 1 of 7 linked papers with an AI index.

activity
20242026
collaborators

7 papers

astro-ph.HE2026

Temporal Memory in Repeating Fast Radio Bursts: Epsilon-Machine Reconstruction of Causal Structure in Burst Timing

Tom Kimpson, Joseph O'Leary

The study applies ε‑machine reconstruction to the burst arrival times of repeating fast radio bursts, showing that two repeaters exhibit about one bit of temporal memory while a th…

gr-qc2026

Search for continuous gravitational waves from neutron stars in five globular clusters in the first part of the fourth LIGO-Virgo-KAGRA observing run

Damon H. T. Cheung, Keith Riles, Rafel Amengual +14

We present the results of directed searches for continuous gravitational waves from unknown neutron stars in five Milky Way globular clusters. We carry out the searches in the LIGO…

astro-ph.HE2026

Discovering pulsars in compact binaries with a hidden Markov model

Joseph O'Leary, Liam Dunn, Andrew Melatos

Discovering radio pulsars in compact binaries, whose orbital periods satisfy , is computationally challenging, because the time-depend…

astro-ph.HE2025

Is there a retrograde accretion disk around 4U 162667? Tracking torque reversals with a state-space model

Joseph O'Leary, Andrew Melatos, Tom Kimpson +5

X-ray timing studies of the persistent, Galactic, accretion-powered pulsar 4U 162667 reveal torque reversals, during which the pulse frequency alternates between multiye…

astro-ph.HE2025

Observing Rayleigh-Taylor stable and unstable accretion through a Kalman filter analysis of X-ray pulsars in the Small Magellanic Cloud

Joseph O'Leary, Andrew Melatos, Tom Kimpson +5

Global, three-dimensional, magnetohydrodynamic simulations of Rayleigh-Taylor instabilities at the disk-magnetosphere boundary of rotating, magnetized, compact stellar objects reve…

astro-ph.IM2025

State-space algorithm for detecting the nanohertz gravitational wave background

Tom Kimpson, Andrew Melatos, Joseph O'Leary +11

The stochastic gravitational wave background (SGWB) can be observed in the nanohertz band using a pulsar timing array (PTA). Here a computationally efficient state-space framework…