activity
20072026
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 9.5k across the 93 of their papers we have counts for

collaborators

94 papers

astro-ph.CO2026

An improved standardization framework for Type II-P supernovae using a hierarchical Bayesian approach

A. Holas, S. Taubenberger, C. Vogl +41

We use Type II-P supernovae (SNe II-P) observed as part of the Nearby Supernova Factory (SNfactory) experiment as standardizable candles to develop an improved standardization fram…

astro-ph.SR2026

Progress towards a 3D Monte Carlo radiative transfer code for outflow wind modelling: II. 3-D applications

Jakub Fišák, Jiří Kubát, Nicolas Moens +1

The massive hot stars play crucial role in the dynamics of galaxies. These stars influence their surroundings through strong winds which are highly structured processes. The theore…

astro-ph.SR2024★ 1 cited

Non-LTE radiative transfer simulations: Improved agreement of the double detonation with normal Type Ia supernovae

Christine E. Collins, Luke J. Shingles, Stuart A. Sim +6

The double detonation is a widely discussed explosion mechanism for Type Ia supernovae, whereby a helium shell detonation ignites a secondary detonation in the carbon/oxygen core o…

astro-ph.HE2024★ 4 cited

Including a Luminous Central Remnant in Radiative Transfer Simulations for Type Iax Supernovae

F. P. Callan, S. A. Sim, C. E. Collins +6

Type Iax supernovae (SNe Iax) are proposed to arise from deflagrations of Chandrasekhar mass white dwarfs (WDs). Previous deflagration simulations have achieved good agreement with…

astro-ph.SR2023★ 14 cited

Helium as a signature of the double detonation in Type Ia supernovae

Christine E. Collins, Stuart A. Sim, Luke. J. Shingles +5

The double detonation is a widely discussed mechanism to explain Type Ia supernovae from explosions of sub-Chandrasekhar mass white dwarfs. In this scenario, a helium detonation is…

astro-ph.SR2022★ 4 cited

Progress towards a 3D Monte Carlo radiative transfer code for outflow wind modelling

Jakub Fišák, Jiří Kubát, Brankica Kubátová +2

Context: Radiative transfer modelling of expanding stellar envelopes is an important task in their analysis. To account for inhomogeneities and deviations from spherical symmetry,…