activity
19972026
most citedGaia Data Release 2. Summary of the contents and survey properties

8.6k citations · 16.1k across the 123 of their papers we have counts for

collaborators

124 papers

astro-ph.IM2026★ 8 cited

Quasi-automatic software support for Gaia ground based optical tracking

S. Bouquillon, C. Barache, T. Carlucci +6

The ESA Gaia satellite mission will create a catalog of 1 billion stars with unprecedented astrometric precision. To achieve its aim in terms of astrometric precision, a ground bas…

astro-ph.IM2026★ 15 cited

GBOT: ground based optical tracking of the Gaia satellite

Martin Altmann, Sebastien Bouquillon, Francois Taris +6

Gaia, the 1 billion star, high precision, astrometric satellite will revolutionise our understanding in many areas of astronomy ranging from bodies in our Solar System to the forma…

astro-ph.HE2023

Optimising the observation of optical kilonovae with medium size telescopes

A. E. Camisasca, I. A. Steele, M. Bulla +2

We consider the optimisation of the observing strategy (cadence, exposure time and filter choice) using medium size (2-m class) optical telescopes in the follow-up of kilonovae loc…

astro-ph.HE2023

GRB 210619B: first gamma-ray burst detection by the novel polarimeter MOPTOP

M. Shrestha, I. A. Steele, S. Kobayashi +4

GRB~210619B was a bright long gamma-ray burst (GRB) which was optically followed up by the novel polarimeter MOPTOP on the Liverpool Telescope (LT). This was the first GRB detectio…

astro-ph.SR2023★ 16 cited

A flash of polarized optical light points to an aspherical "cow"

J. R. Maund, P. A. Hoeflich, I. A. Steele +8

The astronomical transient AT2018cow is the closest example of the new class of luminous, fast blue optical transients (FBOTs). Liverpool Telescope RINGO3 observations of AT2018cow…

astro-ph.IM2022★ 211 cited

The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

Shoko Jin, Scott C. Trager, Gavin B. Dalton +212

WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree…