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20212026
most citedThe cosmological dependence of halo and galaxy assembly bias

29 citations · 79 across the 14 of their papers we have counts for

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Showing 2024Show all

6 papers · 1 filter

astro-ph.CO2024★ 3 cited

FLAMINGO: Galaxy formation and feedback effects on the gas density and velocity fields

Lurdes Ondaro-Mallea, Raul E. Angulo, Giovanni Aricò +3

Most of the visible matter in the Universe is in a gaseous state, subject to hydrodynamic forces and galaxy formation processes that are much more complex to model than gravity. Th…

astro-ph.CO2024★ 4 cited

A 1% accurate method to include baryonic effects in galaxy-galaxy lensing models

Matteo Zennaro, Giovanni Aricò, Carlos García-García +6

Galaxy clustering and galaxy-galaxy lensing are two of the main observational probes in Stage-IV large-scale structure surveys. Unfortunately, the complicated relationship between…

astro-ph.CO2024★ 10 cited

Investigating the galaxy-halo connection of DESI Emission-Line Galaxies with SHAMe-SF

Sara Ortega-Martinez, Sergio Contreras, Raul E. Angulo +1

The Dark Energy Spectroscopic Instrument (DESI) survey is mapping the large-scale distribution of millions of Emission Line Galaxies (ELGs) over vast cosmic volumes to measure the…

astro-ph.CO2024★ 5 cited

FLAMINGO: combining kinetic SZ effect and galaxy-galaxy lensing measurements to gauge the impact of feedback on large-scale structure

Ian G. McCarthy, Alexandra Amon, Joop Schaye +13

Energetic feedback processes associated with accreting supermassive black holes can expel gas from massive haloes and significantly alter various measures of clustering on ~Mpc sca…

astro-ph.GA2024★ 9 cited

Validating the clustering predictions of empirical models with the FLAMINGO simulations

Sergio Contreras, Raul E. Angulo, Jonás Chaves-Montero +3

Context. Mock galaxy catalogues are essential for correctly interpreting current and future generations of galaxy surveys. Despite their significance in galaxy formation and cosmol…

astro-ph.CO2024★ 12 cited

SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model

Sara Ortega-Martinez, Sergio Contreras, Raul Angulo

With the advent of several galaxy surveys targeting star-forming galaxies, it is important to have models capable of interpreting their spatial distribution in terms of astrophysic…