activity
20222026
most citedThe wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

211 citations · 263 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2026

CAVITY: Calar Alto Void Integral-field Treasury surveY: II. Second public data release

B. Bidaran, A. Jiménez, R. García-Benito +30

Studying galaxy evolution under the unique environmental conditions of cosmic voids provides an opportunity to disentangle the role of the large-scale environment in shaping mass a…

astro-ph.GA2026

ALMA CO-CAVITY II. Resolved Scaling Relations in Void Galaxies

S. B. De Daniloff, D. Espada, S. Duarte Puertas +22

Scaling relations involving star formation rates (SFRs), molecular gas mass, and stellar mass are key to understand galaxy evolution, and have previously been explored at resolved…

astro-ph.GA2026★ 1 cited

The CAVITY project. The spatially resolved SFR of galaxies in voids

Ana M. Conrado, Rubén García-Benito, Rosa M. González Delgado +24

The mass in the Universe is distributed non-uniformly, originating the Large Scale Structure (LSS), characterised by clusters, filaments, walls and voids. Galaxies in voids are blu…

astro-ph.GA2025★ 4 cited

Spatially resolved stellar populations and emission lines properties in nearby galaxies with J-PLUS -- I. Method and first results for the M101 group

J. Thainá-Batista, R. Cid Fernandes, R. M. González Delgado +20

Spatially resolved maps of stellar populations and nebular emission are key tools for understanding the physical properties and evolutionary stages of galaxies. We aim to character…

astro-ph.GA2024

CAVITY: Calar Alto Void Integral-field Treasury surveY. I. First public data release

Rubén García-Benito, Andoni Jiménez, Laura Sánchez-Menguiano +40

The Calar Alto Void Integral-field Treasury surveY (CAVITY) is a legacy project aimed at characterising the population of galaxies inhabiting voids, which are the most under-dense…

astro-ph.GA2024★ 7 cited

The effect of local and large scale environment on the star formation histories of galaxies

G. Torres-Ríos, I. Pérez, S. Verley +15

We aim to investigate how the local environment influences the star formation history (SFH) of galaxies residing in various large-scale environments. We categorise a sample of 9384…

astro-ph.GA2024★ 19 cited

CAVITY, Calar Alto Void Integral-field Treasury surveY and project extension

I. Pérez, S. Verley, L. Sánchez-Menguiano +58

We have learnt in the last decades that the majority of galaxies belong to high density regions interconnected in a sponge-like fashion. This large-scale structure is characterised…

astro-ph.GA2024★ 2 cited

Exploring Galaxy Properties of eCALIFA with Contrastive Learning

G. Martínez-Solaeche, R. García-Benito, R. M. González Delgado +4

Contrastive learning (CL) has emerged as a potent tool for building meaningful latent representations of galaxy properties across a broad spectrum of wavelengths, ranging from opti…

astro-ph.GA2024★ 19 cited

The CAVITY project. The spatially resolved stellar population properties of galaxies in voids

Ana M. Conrado, Rosa M. González Delgado, Rubén García-Benito +28

The Universe is shaped as a web-like structure, formed by clusters, filaments, and walls that leave large volumes in between named voids. Galaxies in voids have been found to be of…

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…