activity
20242026
collaborators

33 papers

astro-ph.GA2026

Neighbors, Not Kin: Kinematic evidence for tidal tails from NGC 7492 along the Sagittarius stream

Camila Navarrete, Álvaro Rojas-Arriagada, Andrés E. Piatti +8

The formation, extension, and morphology of extra-tidal stars around globular clusters depend on the internal kinematics of the host cluster and the Galactic potential. Tracing the…

astro-ph.GA2026

Constraining the population of dark matter halo shapes using hierarchical inference with extragalactic stellar streams

David Chemaly, Elisabeth Sola, Vasily Belokurov +4

Stellar streams, the debris of tidally disrupted satellites, trace their host's gravitational potential and thus probe dark matter halo structure. While six-dimensional phase-space…

astro-ph.GA2026

Constraints on the population level distribution of nearby Dark Matter halo shapes with extragalactic streams

David Chemaly, Elisabeth Sola, Sergey Koposov +3

Stellar streams trace the gravitational potential of their host galaxies and provide a sensitive probe of dark matter halo structure. Previously, we developed, and tested on simula…

astro-ph.GA2026

Globular cluster abundance patterns inherited from giant molecular clouds

William McClymont, Vasily Belokurov, Sandro Tacchella +16

Globular clusters exhibit large star-to-star variations and anticorrelations in their light element abundances that are commonly interpreted in terms of in-cluster self-enrichment,…

astro-ph.GA2026

SchwarMAX: a GPU-friendly Schwarzschild orbit-superposition modelling framework

HanYuan Zhang, David Chemaly, Eugene Vasiliev +3

The Schwarzschild orbit-superposition method is a highly flexible dynamical modelling tool. It constrains the mass distribution of a galaxy using line-of-sight velocity and photome…

astro-ph.CO2026

A hierarchical Bayesian framework for cosmology using Type 1 AGN variability

Júlia Laguna-Miralles, Vasily Belokurov, Miles Cranmer

Independent luminosity-distance probes beyond the Type Ia supernova range are needed to test cosmic expansion at high redshift. Type 1 AGN are abundant at \(z>2\), but their use fo…