429 citations · 4.1k across the 77 of their papers we have counts for
13 papers · 1 filter
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…
The large-scale structure around the Fornax-Eridanus Complex
Maria Angela Raj, Petra Awad, Reynier F. Peletier +7
Our objectives are to map the filamentary network around the Fornax-Eridanus Complex and probe the influence of the local environment on galaxy morphology. We employ the novel mach…
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…
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…
Star Formation and Dust in the Cosmic Web
Massimiliano Parente, Cinthia Ragone-Figueroa, Pablo López +8
The large-scale environment of the cosmic web is believed to impact galaxy evolution, but there is still no consensus regarding the mechanisms. We use a semi-analytic model (SAM) g…
Stellar mass-metallicity relation throughout the large-scale structure of the Universe: CAVITY mother sample
Jesús Domínguez-Gómez, Isabel Pérez, Tomás Ruiz-Lara +21
Void galaxies are essential for understanding the physical processes that drive galaxy evolution because they are less affected by external factors than galaxies in denser environm…
Galaxies in voids assemble their stars slowly
J. Domínguez-Gómez, I. Pérez, T. Ruiz-Lara +20
Galaxies in the Universe are distributed in a web-like structure characterised by different large-scale environments: dense clusters, elongated filaments, sheetlike walls, and unde…
CO-CAVITY pilot survey: Molecular gas and star formation in void galaxies
J. Domínguez-Gómez, U. Lisenfeld, I. Pérez +9
We present the first molecular gas mass survey of void galaxies. We compare these new data together with data for the atomic gas mass and star formation rate () from the l…
The Void Galaxy Survey: Photometry, structure and identity of void galaxies
B. Beygu, R. F. Peletier, J. M. van der Hulst +5
We analyze photometry from deep B-band images of 59 void galaxies in the Void Galaxy Survey (VGS), together with their near-infrared 3.6m and 4.5m Spitzer photometry. The VGS…
The Void Galaxy Survey: Star Formation Properties
B. Beygu, K. Kreckel, J. M. van der Hulst +5
We study the star formation properties of 59 void galaxies as part of the Void Galaxy Survey (VGS). Current star formation rates are derived from and recent star formatio…
The Void Galaxy Survey: Morphology and Star Formation Properties of Void Galaxies
B. Beygu, K. Kreckel, J. M. van der Hulst +5
We present the structural and star formation properties of 59 void galaxies as part of the Void Galaxy Survey (VGS). Our aim is to study in detail the physical properties of these…
The Void Galaxy Survey: Galaxy Evolution and Gas Accretion in Voids
Kathryn Kreckel, Jacqueline H. van Gorkom, Burcu Beygu +4
Voids represent a unique environment for the study of galaxy evolution, as the lower density environment is expected to result in shorter merger histories and slower evolution of g…
The metallicity of void dwarf galaxies
K. Kreckel, K. Croxall, B. Groves +2
The current Lambda CDM cosmological model predicts that galaxy evolution proceeds more slowly in lower density environments, suggesting that voids are a prime location to search fo…