2 papers
astro-ph.CO2026
Non-Separable Halo Bias from High-Redshift Galaxy Clustering
Emy Mons, Vipul Prasad Maranchery, M. S. Suryan Sivadas +1
The halo model provides a powerful framework for interpreting galaxy clustering by linking the spatial distribution of dark matter haloes to the underlying matter distribution. A k…
astro-ph.CO2025
Probing Environmental Dependence of High-Redshift Galaxy Properties with the Marked Correlation Function
Emy Mons, Charles Jose
In hierarchical structure formation, correlations between galaxy properties and their environments reveal important clues about galaxy evolution, emphasizing the importance of meas…