activity
20072024
most citedNon-linear structure formation and the acoustic scale

153 citations · 273 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2024★ 23 cited

Analytical and EZmock covariance validation for the DESI 2024 results

Daniel Forero-Sánchez, Michael Rashkovetskyi, Otávio Alves +44

The estimation of uncertainties in cosmological parameters is an important challenge in Large-Scale-Structure (LSS) analyses. For standard analyses such as Baryon Acoustic Oscillat…

astro-ph.CO2023★ 3 cited

The DESI One-Percent survey: exploring the Halo Occupation Distribution of Emission Line Galaxies with AbacusSummit simulations

Antoine Rocher, Vanina Ruhlmann-Kleider, Etienne Burtin +50

The One-Percent survey of the Dark Energy Spectroscopic Instrument collected ~ 270k emission line galaxies (ELGs) at 0.8 < z < 1.6. The high completeness of the sample allowed the…

hep-ex2020★ 48 cited

Search for sterile neutrino oscillation using RENO and NEOS data

Z. Atif, J. H. Choi, B. Y. Han +43

We present a reactor model independent search for sterile neutrino oscillation using 2\,509\,days of RENO near detector data and 180 days of NEOS data. The reactor related systemat…

hep-ex2020★ 26 cited

Search for Sub-eV Sterile Neutrino at RENO

The RENO Collaboration, J. H. Choi, H. I. Jang +25

We report a search result for a light sterile neutrino oscillation with roughly 2200 live days of data in the RENO experiment. The search is performed by electron antineutrino ($\o…

astro-ph2008★ 153 cited

Non-linear structure formation and the acoustic scale

Hee-Jong Seo, Ethan R. Siegel, Daniel J. Eisenstein +1

We present high signal-to-noise measurements of the acoustic scale in the presence of nonlinear growth and redshift distortions using 320(Gpc/h)^3 of cosmological PM simulations. U…

astro-ph2007★ 20 cited

Passive Evolution of Galaxy Clustering

Hee-Jong Seo, Daniel J. Eisenstein, Idit Zehavi

We present a numerical study of the evolution of galaxy clustering when galaxies flow passively from high redshift, respecting the continuity equation throughout. While passive flo…