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

1 citations · 1 across the 3 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2026

Magnetar counterparts, kinematics and birth sites with HST and JWST

A. A. Chrimes, J. D. Lyman, A. J. Levan +7

Magnetars are highly magnetised, isolated neutron stars with uncertain formation channels. They comprise a potentially significant fraction of the young neutron star population in…

astro-ph.CO2026

The local ultraviolet signature of Type Ia supernova environments from HST and MUSE

Lluís Galbany, Cullen Abelson, Alaa Alburai +17

(Abridged.) The local environment of a Type Ia supernova (SN Ia) encodes information on progenitor age, star formation, dust, and chemical enrichment that may influence both its li…

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.HE2026

GOTO identification and broadband modelling of the counterpart to the SVOM GRB 250818B

S. Belkin, G. P. Lamb, K. Ackley +61

Rapid localisation and follow-up of gamma-ray bursts (GRBs) increasingly rely on low-latency triggers from new missions coupled to wide-field robotic optical facilities. We present…

astro-ph.IM2025

A search for photometric variability towards the globular cluster M3 with the TWenty Inch Survey Telescope

Morgan A. Mitchell, Paul Chote, James McCormac +9

We present the commissioning results and first scientific observations from the newly installed TWIST observatory - a 50 cm telescope equipped with an sCMOS camera providing a $36.…

astro-ph.HE2025

MUSE Observations Reveal Optical Coronal Iron Lines from Shock Emission in Supernova Remnant 0540-69.3

L. Tenhu, J. Larsson, P. Lundqvist +3

We investigate the optical shock emission from the Large Magellanic Cloud supernova remnant 0540-69.3 (SNR 0540) using MUSE integral-field-unit data from the VLT. The observations…