collaborators

6 papers

astro-ph.HE2026

Understanding the Neutron Star Population with the SKAO Telescopes

L. Levin, M. Bagchi, M. Burgay +12

The known population of non-accreting neutron stars is ever growing and currently consists of more than 3500 sources. Pulsar surveys with the SKAO telescopes will greatly increase…

astro-ph.SR2026

An interferometric study of B star multiplicity

A. J. Frost, H. Sana, J-B Le Bouquin +7

Massive stars can have extreme effects on their environments from local to galactic scales. While O star multiplicity has been studied over a broad separation range (to the point w…

astro-ph.HE2026

Population synthesis predictions of the Galactic compact binary gravitational wave foreground detectable by LISA

Jake McMillan, Adam Ingram, Cordelia Dashwood Brown +4

We use population synthesis modelling to predict the gravitational wave (GW) signal that the Laser Interferometer Space Antenna (LISA) will detect from the Galactic population of c…

astro-ph.HE2026

Probing the millisecond pulsar origin of the -ray excess in the Galactic centre with LISA

Valeriya Korol, Andrei Igoshev

The gigaelectronvolt -ray excess observed towards the Galactic centre remains unexplained. While dark matter annihilation has long been considered a leading explanation, an alt…

astro-ph.HE2025

Understanding the Neutron Star Population with the SKAO telescopes

L. Levin, M. Bagchi, M. Burgay +13

The known population of non-accreting neutron stars is ever growing and currently consists of more than 3500 sources. Pulsar surveys with the SKAO telescopes will greatly increase…

astro-ph.HE2025

From proto-neutron star dynamo to low-field magnetars

Andrei Igoshev, Paul Barrère, Raphaël Raynaud +3

Low-field magnetars have dipolar magnetic fields that are 10-100 times weaker than the threshold, G, used to define classical magnetars, yet they produce simila…