activity
20122026
most citedThe wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

211 citations · 343 across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2026

The Gas-Phase Mass-Metallicity Relation of Dwarf Galaxies Across Large-Scale Environments Using the CAVITY Parent Sample

Bahar Bidaran, Salvador Duarte Puertas, Isabel Pérez +13

The gas-phase mass-metallicity relation (MZR) of galaxies shows a noticeable break in slope and increased scatter at low stellar masses, suggesting that the physical processes gove…

astro-ph.GA2026

Galaxy groups within voids

M. Argudo-Fernández, G. Torres-Ríos, P. Vásquez-Bustos +18

In this work, we aim to identify and characterise a sample of galaxy groups within voids in the local Universe (z\,<\,0.08), taking into account the peculiarities of these vast and…

astro-ph.GA2026

ALMA CO-CAVITY I. Resolved Molecular Gas in Void Galaxies

D. Espada, S. B. De Daniloff, S. Duarte Puertas +21

The environment plays a key role in galaxy evolution, yet it remains unclear how detailed molecular gas properties and their connection to star formation and stellar content are in…

astro-ph.GA2025★ 4 cited

Rendezvous in CAVITY: Kinematics and gas properties of an isolated dwarf-dwarf merging pair in a cosmic void region

Bahar Bidaran, Simon de Daniloff, Isabel Pérez +17

Galaxy mergers are pivotal events in the evolutionary history of galaxies, with their impact believed to be particularly significant in dwarf galaxies. We report the serendipitous…

astro-ph.GA2025

MeerKAT view of Hickson Compact Groups: II. HI deficiency in the core and surrounding regions

A. Sorgho, L. Verdes-Montenegro, R. Ianjamasimanana +25

Hickson compact groups (HCGs) offer an ideal environment for investigating galaxy transformation as a result of interactions. It has been established that the evolutionary sequence…

astro-ph.GA2025★ 2 cited

MeerKAT view of Hickson Compact Groups:I. Data description and release

R. Ianjamasimanana, L. Verdes-Montenegro, A. Sorgho +25

Context: Hickson Compact Groups (HCGs) are dense gravitationally-bound collections of 4-10 galaxies ideal for studying gas and star formation quenching processes. Aims: We aim to u…

astro-ph.IM2024

Interactive Multimodal Integral Field Spectroscopy

Adrián García Riber, Rubén García-Benito, Francisco Serradilla

Using sonification on scientific data analysis provides additional dimensions to visualization, potentially increasing researchers' analytical capabilities and fostering inclusion…

astro-ph.GA2024

PGC 44685: A Dwarf Star-forming Lenticular Galaxy with Wolf-Rayet Population

Shiying Lu, Qiusheng Gu, Yulong Gao +8

Lenticular galaxies (S0s) are formed mainly from the gas stripping of spirals in the cluster. But how S0s form and evolve in the field is still untangled. Based on spatially resolv…

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.GA2023★ 2 cited

Supernova environments in J-PLUS. Normalized Cumulative Rank distributions and stellar population synthesis, combining narrow- and broad-band filters

Raul González-Díaz, Lluís Galbany, Tuomas Kangas +26

We study the local environmental properties of 418 supernovae (SNe) of all types using data from the Javalambre Photometric Local Universe Survey (J-PLUS), which includes 5 broad-…

astro-ph.GA2023★ 5 cited

Assessing model-based carbon and oxygen abundance derivation from ultraviolet emission lines in AGNs

Enrique Pérez-Montero, Ricardo Amorín, Borja Pérez-Díaz +2

We present an adapted version of the code HII-CHI-Mistry-UV (Pérez-Montero & Amorín 2017) to derive chemical abundances from emission lines in the ultraviolet, for use in narrow li…

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.IM2022★ 7 cited

Painting graphs with sounds: CosMonic sonification project

Rubén García-Benito, Enrique Pérez-Montero

CosMOnic (COSmos harMONIC) is a sonification project with a triple purpose: analysis (by means of sounds) of any type of data, source of inspiration for artistic creations, and ped…

astro-ph.GA2021

Galaxy evolution on resolved scales: ageing and quenching in CALIFA

Pablo Corcho-Caballero, Javier Casado, Yago Ascasibar +1

This work investigates the fundamental mechanism(s) that drive galaxy evolution in the Local Universe. By comparing two proxies of star-formation sensitive to different timescales,…

astro-ph.GA2016★ 19 cited

The SELGIFS data challenge: generating synthetic observations of CALIFA galaxies from hydrodynamical simulations

Giovanni Guidi, Javier Casado, Yago Ascasibar +6

In this work we present a set of synthetic observations that mimic the properties of the Integral Field Spectroscopy (IFS) survey CALIFA, generated using radiative transfer techniq…

astro-ph.IM2016★ 8 cited

BaTMAn: Bayesian Technique for Multi-image Analysis

J. Casado, Y. Ascasibar, R. García-Benito +5

This paper describes the Bayesian Technique for Multi-image Analysis (BaTMAn), a novel image-segmentation technique based on Bayesian statistics that characterizes any astronomical…

astro-ph.GA2015★ 45 cited

Towards a new classification of galaxies: principal component analysis of CALIFA circular velocity curves

Veselina Kalinova, Dario Colombo, Erik Rosolowsky +16

We present a galaxy classification system for 238 (E1-Sdm) CALIFA (Calar Alto Legacy Integral Field Area) galaxies based on the shapes and amplitudes of their circular velocity cur…

astro-ph.CO2012★ 21 cited

Auto-consistent metallicity and star formation history of the nearest blue compact dwarf galaxy NGC 6789

Rubén García-Benito, Enrique Pérez-Montero

We present a detailed auto-consistent study of the nearest blue compact dwarf galaxy NGC 6789 by means of optical and UV archive photometry data and optical long-slit ISIS-WHT spec…