most citedThe Gravitational-wave Optical Transient Observer (GOTO) data pipeline and workflow for transient discovery

1 citations · 1 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2026

The progenitors and circumstellar environments of stripped-envelope interacting supernovae from BPASS

B. Warwick, J. Lyman, D. L. Coppejans +4

Understanding the progenitors of stripped-envelope interacting supernovae (SEISNe) is crucial for probing the final stages of massive star evolution. Despite this, their rarity mea…

astro-ph.IM20261 cited

The Gravitational-wave Optical Transient Observer (GOTO) data pipeline and workflow for transient discovery

J. D. Lyman, D. O'Neill, T. Killestein +45

Wide-field and high-cadence sky surveys are the first step in the chain of discovery and characterisation of astrophysical transients such as supernovae, kilonovae, and tidal disru…

astro-ph.IM2026

Where to Search For Life: Evidence from narrative sources with established predictive efficacy

Elizabeth R Stanway

The search for habitable planets, and even for ``Earth 2.0'', is a major driver in contemporary astronomy. However selecting target fields to prioritise for such searches presents…

astro-ph.GA2025

Impact of Uncertainties in Spectral Energy Distribution Modelling on Inferred Galaxy Properties

Gareth T. Jones, Conor M. Byrne, Elizabeth R. Stanway

Interpreting galaxy properties from astronomical surveys relies heavily on spectral energy distribution (SED) modelling, yet uncertainties in key model ingredients are often overlo…

astro-ph.HE2025

X-BPASS : Self-consistent modelling of stellar populations and their associated X-ray Binary emission in a binary stellar evolution framework

J. C. Bray, E. R. Stanway, J. J. Eldridge

X-ray binaries play a significant role in the thermal and ionization history of galaxies. Their X-ray luminosity can shed light on galactic star formation rates and histories. Comp…

astro-ph.GA2025

What do we mean by stellar mass? The impact of the pre-main sequence on the mass to light ratio of young and intermediate age stellar populations

Elizabeth R. Stanway, Conor M. Byrne, Ankur Upadhyaya

Stellar population synthesis models are an essential tool with which galaxy physical parameters are extracted from observations. However they are built on assumptions designed for…