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20112026
most citedCompact Remnant Mass Function: Dependence on the Explosion Mechanism and Metallicity

1k citations · 1.8k across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.HE2026

COBALT-BLUE: a fast and accurate model for gravitational self-lensing binary systems

Danny J. Dixon, Adam Ingram, Matthew J. Middleton +5

We present COBALT-BLUE, a fast public model for the optical light curve of a luminous star in a non-accreting binary with a compact object. The model includes gravitational self-le…

astro-ph.GA2023★ 6 cited

Synthetic Population of Binary Cepheids. II. The effect of companion light on the extragalactic distance scale

Paulina Karczmarek, Gergely Hajdu, Grzegorz Pietrzyński +5

Because of their period-luminosity relation (PLR), classical Cepheids play a key role in the calibration of the extragalactic distance scale and the determination of the Hubble-Lem…

astro-ph.SR2022★ 10 cited

Synthetic population of binary Cepheids. I. The effect of metallicity and initial parameter distribution on characteristics of Cepheids' companions

Paulina Karczmarek, Radosław Smolec, Gergely Hajdu +5

The majority of classical Cepheids are binary stars, yet the contribution of companions' light to the total brightness of the system has been assumed negligible and lacked a thorou…

astro-ph.HE2021★ 8 cited

The impact of precession on the observed population of ULXs

Norman Khan, Matthew. J. Middleton, Grzegorz Wiktorowicz +3

The discovery of neutron stars powering several ultraluminous X-ray sources (ULXs) raises important questions about the nature of the underlying population. In this paper we build…

astro-ph.HE2021★ 19 cited

Thermally driven winds in ULXs

Matthew Middleton, Nick Higginbottom, Christian Knigge +2

The presence of radiatively driven outflows is well established in ultraluminous X-ray sources (ULXs). These outflows are optically thick and can reprocess a significant fraction o…

astro-ph.HE2021★ 18 cited

Predicting the self-lensing population in optical surveys

Grzegorz Wiktorowicz, Matthew Middleton, Norman Khan +3

The vast majority of binaries containing a compact object and a regular star spend most of their time in a quiescent state where no strong interactions occur between components. De…