collaborators

6 papers

astro-ph.HE2026

nDspec: a new Python library for modelling multi-dimensional datasets in X-ray astronomy

Matteo Lucchini, Benjamin Ricketts, Phil Uttley +1

The current fleet of X-ray telescopes produces a wealth of multi-dimensional data, allowing us to study sources in time, photon energy, and polarisation. At the same time, it has b…

astro-ph.IM2026

Emulation of non-linear 1D spectral models: relativistic X-ray reflection

Benjamin J. Ricketts, Tin Hadži Veljković, Daniela Huppenkothen +4

The use of machine learning techniques to approximate computationally expensive models has become increasingly prevalent in a wide variety of fields within astronomy. We discuss th…

astro-ph.SR2026

Pushing the Limit of Asteroseismic Detection for Cool Dwarfs using TESS and Deep Learning

Waly M Z Karim, Rocio Kiman, Derek Buzasi +6

Asteroseismology provides a powerful probe of stellar interiors by detecting stellar oscillations, including solar-like oscillations, which are stochastically excited by near-surfa…

astro-ph.HE2026

Disk warping and black hole X-ray binaries I. Tentative unification of low-frequency quasi-periodic oscillations

Gregoire Marcel, Samuel Turner, Benjamin Ricketts +6

X-ray binaries exhibit complex variability patterns studied in the power-spectrum. These include the broad-band noise (BBN) components and various types of narrow components called…

astro-ph.HE2026

Equation-of-state-informed pulse profile modeling

Mariska Hoogkamer, Nathan Rutherford, Daniela Huppenkothen +9

NICER has enabled mass-radius inferences for pulsars using pulse profile modeling (PPM), providing constraints on the equation of state (EOS) of cold, dense matter. To date, PPM an…

astro-ph.HE2025

RTFAST-Spectra: Emulation of X-ray reverberation mapping for active galactic nuclei

Benjamin Ricketts, Daniela Huppenkothen, Matteo Lucchini +4

Bayesian analysis has begun to be more widely adopted in X-ray spectroscopy, but it has largely been constrained to relatively simple physical models due to limitations in X-ray mo…