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20222026
most citedSHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model

12 citations · 32 across the 7 of their papers we have counts for

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5 papers · 1 filter

astro-ph.CO2026

Validation of the Hybrid Bias Expansion model for the galaxy bispectrum

Marcos Pellejero Ibáñez, Raul E. Angulo, Laila Linke +8

The Hybrid Bias Expansion model (also known as Hybrid Effective Field Theory, HEFT) provides a promising way to extend the range of validity of perturbative large-scale structure m…

astro-ph.CO2026

Cosmological constraints from the small scale clustering of Emission Line Galaxies

Sara Ortega-Martinez, Raul E. Angulo, Sergio Contreras +7

Spectroscopic surveys such as the Dark Energy Spectroscopic Instrument (DESI) and Euclid are mapping the spatial distribution of millions of galaxies, with Emission Line Galaxies (…

astro-ph.CO2025

Illuminating the Physics of Dark Energy with the Discovery Simulations

Gillian D. Beltz-Mohrmann, Adrian Pope, Alex Alarcon +10

In this paper, we present the Discovery simulations: a new pair of high-resolution N-body simulations motivated by the DESI Y1 BAO cosmological constraints on dark energy. The Disc…

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★ 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…