collaborators

6 papers

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

A NICER view of the 1.4 solar-mass edge-on pulsar PSR J0614-3329

Lucien Mauviard, Sebastien Guillot, Tuomo Salmi +20

Four neutron star radius measurements have already been obtained by modeling the X-ray pulses of rotation-powered millisecond pulsars observed by the Neutron Star Interior Composit…

astro-ph.HE2025

The variability of active galaxies: I. Broad-band noise X-ray power spectra from XMM-Newton and Swift

Mehdy Lefkir, Simon Vaughan, Mike Goad +2

Accreting supermassive black holes at the centres of galaxies are the engine of active galactic nuclei (AGN). X-ray light curves of unabsorbed AGN show dramatic random variability…

astro-ph.HE2025

Searching for quasi-periodicities in short transients: the curious case of GRB 230307A

Daniela Huppenkothen, Matthew G. Baring, Mete Uzuner +5

Gamma-ray bursts (GRBs) are the most powerful explosions in the Universe; their energy release reache s us from the end of the re-ionization era, making them invaluable cosmologica…

astro-ph.GA2025

Modelling variability power spectra of active galaxies from irregular time series

Mehdy Lefkir, Simon Vaughan, Daniela Huppenkothen +2

A common feature of Active Galactic Nuclei (AGN) is their random variations in brightness across the whole emission spectrum, from radio to -rays. Studying the nature and origi…

astro-ph.HE2025

The Galactic population of magnetars : a simulation-based inference study

Mattéo Sautron, Alexander Eli McEwen, George Younes +3

Population synthesis modeling of the observed dynamical and physical properties of a population is a highly effective method for constraining the underlying birth parameters and ev…