activity
20072022
most citedThe Pan-STARRS1 Surveys

723 citations · 6.3k across the 79 of their papers we have counts for

collaborators

79 papers

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…

astro-ph.GA2022★ 67 cited

The synchronised dance of the Magellanic Clouds' star formation history

P. Massana, T. Ruiz-Lara, N. E. D. Noël +17

We use the SMASH survey to obtain unprecedented deep photometry reaching down to the oldest main sequence turn-offs in the colour-magnitude diagrams (CMDs) of the Small Magellanic…

astro-ph.GA2022★ 8 cited

Forward and Back: Kinematics of the Palomar 5 Tidal Tails

Pete B. Kuzma, Annette M. N. Ferguson, Anna Lisa Varri +5

The tidal tails of Palomar 5 (Pal 5) have been the focus of many spectroscopic studies in an attempt to identify individual stars lying along the stream and characterise their kine…

astro-ph.GA2021★ 20 cited

Variable stars in Local Group Galaxies -- V. The fast and early evolution of the low-mass Eridanus II dSph galaxy

C. E. Martínez-Vázquez, M. Monelli, S. Cassisi +18

We present a detailed study of the variable star population of Eridanus II (Eri II), an ultra-faint dwarf galaxy that lies close to the Milky Way virial radius. We analyze multi-ep…

astro-ph.GA2021★ 39 cited

The star formation history of Eridanus II: on the role of SNe feedback in the quenching of ultra-faint dwarf galaxies

C. Gallart, M. Monelli, T. Ruiz-Lara +17

Eridanus II (EriII) is an ultra-faint dwarf (UFD) galaxy (M_V=-7.1) located at a distance close to the Milky Way virial radius. Early shallow color-magnitude diagrams (CMD) indicat…

astro-ph.GA2020★ 1 cited

"Observations" of simulated dwarf galaxies: Star-formation histories from color-magnitude diagrams

Shivangee Rathi, Michele Mastropietro, Sven De Rijcke +3

Apparent deviations between properties of dwarf galaxies from observations and simulations are known to exist, such as the "Missing Dwarfs" problem, the too-big-to-fail problem, an…