most citedGalaxy mass-size segregation in the cosmic web from the CAVITY parent sample

10 citations · 13 across the 7 of their papers we have counts for

collaborators

7 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

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.CO2025★ 3 cited

The role of supercluster filaments in shaping galaxy clusters

Raúl Baier-Soto, Yara Jaffé, Alexis Finoguenov +44

In a hierarchical CDM Universe, cosmic filaments serve as the primary channels for matter accretion into galaxy clusters, influencing the shape of their dark matter halos. We in…