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

1 citations · 1 across the 4 of their papers we have counts for

collaborators

7 papers

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.GA20261 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.CO2026

Mimicking the large-scale structure of the Local Universe. Synthetic pre-labelled galaxies in large-scale structures

M. Alcázar-Laynez, S. Duarte Puertas, S. Verley +6

Current observational and simulated large-scale structure (LSS) catalogues often lack consistency in assigning galaxies to specific structures, due to the absence of a universally…

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

CO-CAVITY project: Molecular gas and star formation in void galaxies

M. I. Rodríguez, U. Lisenfeld, S. Duarte Puertas +21

Cosmic voids, distinguished by their low-density environment, provide a unique opportunity to explore the interplay between the cosmic environment and the processes of galaxy forma…

astro-ph.GA2024

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…