most citedELGLRG distribution through dark matter halo dynamics

2 citations · 2 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph.CO2026

Cosmic variance or galaxy bias? Disentangling finite-volume and galaxy formation effects in cosmological analysis

Francesco Sinigaglia, Francisco-Shu Kitaura

Current and forthcoming galaxy redshift surveys, such as DESI and Euclid, are going to bring cosmological analysis to an unprecedentedly exquisite level of precision in the determi…

astro-ph.CO2026

HI Simulations for Cosmology with the SKA Observatory

Tommaso Ronconi, Gabriella De Lucia, Marta Spinelli +15

We present a comparative overview of state-of-the-art methods for modelling the distribution of neutral hydrogen (HI) in the post-reionization Universe, developed in preparation fo…

astro-ph.CO2026

Emergence of Complex Web Structures

Francisco-Shu Kitaura

Complex structures often emerge from initially homogeneous or weakly correlated states. We address the apparent tension between this ordering and entropy growth through a unified f…

astro-ph.GA20262 cited

ELGLRG distribution through dark matter halo dynamics

Ginevra Favole, Francisco-Shu Kitaura, Boryana Hadzhiyska +3

We investigate the clustering and halo occupation distribution (HOD) of DESI Y1 emission-line (ELGs) and luminous red (LRGs) galaxies at , including their cross-correlat…

astro-ph.CO2026

Fast and accurate Gaia-unWISE quasar mock catalogs from LPT and Eulerian bias

Francesco Sinigaglia, Francisco-Shu Kitaura, Mahlet Shiferaw +3

We present full-sky quasar spectrophotometric mock catalogs with smooth redshift evolution from to , tailored to analyze the Gaia-unWISE Quasar Catalog (Quaia)…

astro-ph.CO2026

Tracing the high-z cosmic web with Quaia: catalogues of voids and clusters in the quasar distribution

Nestor Arsenov, Andras Kovacs, Mar Perez Sar +5

Understanding the formation and evolution of the cosmic web of galaxies is a fundamental goal of cosmology, using various tracers of the cosmic large-scale structure at an ever wid…