2023/11/21 by Balaguera-Antolínez, Andrés, Montero-Dorta, Antonio D., Favole, Ginevra
#Cosmology and Nongalactic Astrophysics (astro-ph.CO) #FOS: Physical sciences
paper · doi:10.48550/arxiv.2311.12991
We measure the signal of secondary halo bias as a function of a variety of intrinsic and environmental halo properties, and characterize its statistical significance as a function of cosmological redshift. Using fixed and paired N-body simulations of dark-matter halos -- the UNIT simulation -- with masses above 1011M\odoth-1 identified over a wide range of cosmological redshifts (0