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20112026
most citedOverview of the Instrumentation for the Dark Energy Spectroscopic Instrument

465 citations · 1.9k across the 35 of their papers we have counts for

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29 papers · 1 filter

astro-ph.CO2026

Can Fingers of God be Resummed?

Shi-Fan Chen, Alejandro Aviles

Fingers of God (FoGs), Doppler shifts due to the small-scale virial motions of galaxies, are one of the most significant challenges for analytic models of galaxy clustering in reds…

astro-ph.CO2026

Field-level inference of growth rate from DESI BGS galaxy and ZTF supernova simulations

Corentin Ravoux, Bastien Carreres, Julian Bautista +60

Galaxy peculiar velocities are a powerful probe of the growth rate of structure at low redshifts (), measured through the combination . These constraints are imp…

astro-ph.CO2023★ 3 cited

Galaxy bias in the era of LSST: perturbative bias expansions

Andrina Nicola, Boryana Hadzhiyska, Nathan Findlay +14

Upcoming imaging surveys will allow for high signal-to-noise measurements of galaxy clustering at small scales. In this work, we present the results of the LSST bias challenge, the…

astro-ph.CO2023★ 6 cited

Validation of the Scientific Program for the Dark Energy Spectroscopic Instrument

DESI Collaboration, A. G. Adame, J. Aguilar +261

The Dark Energy Spectroscopic Instrument (DESI) was designed to conduct a survey covering 14,000 deg over five years to constrain the cosmic expansion history through precise m…

astro-ph.CO2023★ 8 cited

On the galaxy 3-point correlation function in Modified Gravity

Alejandro Aviles, Gustavo Niz

The next generation of galaxy surveys will provide highly accurate measurements of the large-scale structure of the Universe, allowing for more stringent tests of gravity on cosmol…

astro-ph.CO2023★ 1 cited

Impact of a Rapid Diluted Energy Density on the halo mass function

Dante V. Gomez-Navarro, Alejandro Aviles, Axel de la Macorra

We study dark energy cosmological models, extensions of the standard model of particles, characterized by having an extra relativistic energy density at very early times, and that…