activity
20242026
collaborators

13 papers

astro-ph.CO2026

Intracluster light and dark matter halo shapes reflect common assembly, not mutual coupling: shape correspondence in CDM but not SIDM

G. Martin, N. A. Hatch, W. Cui +8

The intracluster light (ICL) has been proposed as a luminous tracer of the dark matter (DM) halo shape in galaxy clusters, with recent observational studies and CDM simulations…

astro-ph.CO2026

Climbing the -point Ladder Part I: Information in the Higher-Order Configuration-Space Clustering of Dark Matter Halos

Sumi Kim, Cristiano G. Sabiu, Inkyu Park

The two-point correlation function completely describes a Gaussian random field, but nonlinear gravitational growth, halo bias, and redshift-space distortions drive the late-time h…

astro-ph.IM2026

Fast Graph-based Higher-Order Clustering Statistics on the GPU

Cristiano G. Sabiu

We present a significant update to GRAMSCI (GRAph Made Statistics for Cosmological Information; Sabiu et.al 2019), an algorithm for the fast computation of the general -point sp…

astro-ph.GA2026

Groups of Dwarf Galaxies in the Local Universe

Sanjaya Paudel, Cristiano G. Sabiu, Suk-Jin Yoon +3

We present a systematic search for dwarf-galaxy groups in the local Universe (), identifying 28 systems containing at least four spectroscopically confirmed members selecte…

astro-ph.CO2026

Intracluster Light as a Probe for Dark Matter: Exploring SIDM and CDM with C-EAGLE Sims

Jaewon Yoo, Ellen L. Sirks, Cristiano G. Sabiu +5

We assess whether intracluster light (ICL) can serve as an observational discriminator of dark matter physics. The self-interacting dark matter (SIDM) model has gained increasing a…

astro-ph.GA2026

K-DRIFT Science Theme: Galaxies in the Faint Universe

Woowon Byun, Yongmin Yoon, Jongwan Ko +17

Low-surface-brightness (LSB) structures serve as evidence of the intricate mass assembly of galaxies, and dedicatedly studying them promises to give us profound insights into the e…