activity
20242026
collaborators

7 papers

astro-ph.CO2026

Simba Simulation: The Effect of Feedback Physics on Matter Distribution in the Cosmic Web

Chenze Dong, Florian Dedieu, Daniela Galárraga-Espinosa +3

The discrepancy between the early-time estimation and late-time observation on the cosmic baryon content - the 'missing baryon problem' - is a longstanding problem in cosmology. Al…

astro-ph.CO2025

Unveiling the small-scale web around galaxies with miniJPAS and DESI

Daniela Galárraga-Espinosa, Guinevere Kauffmann, Silvia Bonoli +23

We present the first statistical observational study detecting filaments in the immediate surroundings of galaxies, i.e. the local web of galaxies. Simulations predict that cold ga…

astro-ph.GA2025

Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium

Soumya Shreeram, Daniela Galárraga-Espinosa, Johan Comparat +9

The hot circumgalactic medium (CGM), probed by X-ray observations, plays a central role in understanding gas flows that drive a galaxy's evolution. While CGM properties have been w…

astro-ph.GA2025

Central galaxy alignments. Dependence on the mass and the large-scale environment

Facundo Rodriguez, Manuel Merchán, Daniela Galárraga-Espinosa +4

Observations indicate that central galaxies show a significant alignment of their main shape axes with other galaxies in their group, as well as with the large-scale structure of t…

astro-ph.CO2025

The galaxy bias profile of cosmic voids

Antonio D. Montero-Dorta, Andrés Balaguera-Antolínez, Ignacio G. Alfaro +7

Cosmic voids are underdense regions within the large-scale structure of the Universe, spanning a wide range of physical scales - from a few megaparsecs (Mpc) to the largest observa…

astro-ph.GA2025

Pearls on a string: Dark and bright galaxies on a strikingly straight and narrow filament

Maryam Arabsalmani, Sambit Roychowdhury, Benjamin Schneider +11

We identify a chain of galaxies along an almost straight line in the nearby Universe with a projected length of ~5 Mpc. The galaxies are distributed within projected distances of o…