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20242026
most citedELGLRG distribution through dark matter halo dynamics

2 citations · 3 across the 3 of their papers we have counts for

collaborators

7 papers

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.CO20261 cited

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…

astro-ph.CO2026

Differentiable Fuzzy Cosmic-Web for Field Level Inference

P. Rosselló, F. -S. Kitaura, D. Forero-Sánchez +2

A comprehensive analysis of the cosmological large-scale structure derived from galaxy surveys involves field-level inference, which requires a forward modelling framework that sim…

astro-ph.SR2025

New insight into the variability of the Be star Aquarii: Determination of stellar and disk parameters

D. Concha, C. Arcos, D. Turis-Gallo +4

The Be star Aquarii shows peculiar Cas-type X-ray emission, likely caused by its outer disk interacting with a low-mass companion, probably a white dwarf. We study the lo…

astro-ph.CO2024

Exploring the physical origins of halo assembly bias from early times

Antonio D. Montero-Dorta, Sergio Contreras, M. Celeste Artale +2

The large-scale linear halo bias encodes the relation between the clustering of dark-matter (DM) halos and that of the underlying matter density field. Although the primary depende…