activity
20192023
most citedThe wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

211 citations · 327 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2023★ 20 cited

WEAVE-StePS. A stellar population survey using WEAVE at WHT

A. Iovino, B. M. Poggianti, A. Mercurio +44

The upcoming new generation of optical spectrographs on four-meter-class telescopes will provide valuable opportunities for forthcoming galaxy surveys through their huge multiplexi…

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.GA2020★ 39 cited

The S2 Stream: the shreds of a primitive dwarf galaxy

David S. Aguado, G. C. Myeong, Vasily Belokurov +12

The S2 stream is a kinematically cold stream that is plunging downwards through the Galactic disc. It may be part of a hotter and more diffuse structure called the Helmi stream. We…

astro-ph.GA2019★ 28 cited

A few StePS forward in unveiling the complexity of galaxy evolution: light-weighted stellar ages of intermediate redshift galaxies with WEAVE

L. Costantin, A. Iovino, S. Zibetti +29

The upcoming new generation of optical spectrographs on four-meter-class telescopes will provide invaluable information for reconstructing the history of star formation in individu…

astro-ph.GA2019★ 29 cited

Stellar populations of galaxies in the ALHAMBRA survey up to . IV. Properties of quiescent galaxies on the stellar masssize plane

L. A. Díaz-García, A. J. Cenarro, C. López-Sanjuan +7

We perform a comprehensive study of the stellar population properties of quiescent galaxies as a function of size and stellar mass to constrain the physical mechanism governing the…