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20012025
most citedThe wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

211 citations · 1.2k across the 42 of their papers we have counts for

collaborators

42 papers

astro-ph.SR2025★ 4 cited

NGC 663 as a laboratory for massive star evolution

Amparo Marco, Ignacio Negueruela, Norberto Castro +1

Massive young clusters with rich populations of high-mass stars are ideal laboratories to explore their evolutionary paths. Despite being the most prominent cluster in the Perseus-…

astro-ph.SR2024

Astro+: Design, construction, and scientific exploitation of a large-scale massive star spectroscopic database

Klaus Rubke, Amparo Marco, Ignacio Negueruela +4

Massive stars condition the evolution of the interstellar medium by the amount of energy released during their lives and especially by their deaths as supernova explosions. The vas…

astro-ph.IM2022

Web-based telluric correction made in Spain: spectral fitting of Vega-type telluric standards

D. de la Fuente, A. Marco, L. R. Patrick +7

Infrared spectroscopic observations from the ground must be corrected from telluric contamination to make them ready for scientific analyses. However, telluric correction is often…

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.SR2022★ 26 cited

Westerlund 1 under the light of Gaia EDR3: Distance, isolation, extent, and a hidden population

Ignacio Negueruela, Emilio J. Alfaro, Ricardo Dorda +3

(Abridged) We have used Gaia EDR3 data, together with spectra of a large sample of luminous stars in the field surrounding Westerlund 1, to explore the extent of the cluster. We ca…

astro-ph.GA2021★ 7 cited

A massive open cluster hiding in full sight

Ignacio Negueruela, André-Nicolas Chené, Hugo M. Tabernero +4

Obscuration and confusion conspire to limit our knowledge of the inner Milky Way. Even at moderate distances, the identification of stellar systems becomes compounded by the extrem…