activity
20072026
most citedThe Fifth Data Release of the Sloan Digital Sky Survey

744 citations · 3.2k across the 58 of their papers we have counts for

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Showing 2026Show all

14 papers · 1 filter

astro-ph.GA2026

Snapshots of r-process production in the Milky Way disk

Sarah G. Kane, Stephanie Monty, Madeleine McKenzie +9

Stars enhanced in heavy neutron capture elements like europium (Eu) provide a window into the rarest and most exotic nucleosynthetic events. Most Eu-enhanced stars discovered thus…

astro-ph.GA2026

Gone with the wind? Potential gas inflow in the broad-line region of a QSO at traced by time-varying Balmer absorption

Xihan Ji, Dominic J. Walton, Francesco D'Eugenio +6

We report spectroscopic observations of a remarkable QSO, J115724.80-000455.56 at from the Dark Energy Spectroscopic Instrument (DESI) survey. This QSO exhibits variabili…

astro-ph.GA2026

Slow stellar halo rotation as a signature of disc flips and GES-like mergers

Kirill Batrakov, Alis J. Deason, Francesca Fragkoudi +3

The stellar halo of the Milky Way (MW) exhibits a weak net prograde rotational signal ( km~s), yet its origin remains unexplained. To investigate this, we u…

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

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…

astro-ph.GA2026

Self-interacting dark matter promotes bar formation in disk galaxies

Shashank Dattathri, Frank C. van den Bosch, HanYuan Zhang +4

Despite its remarkable success on large scales, the standard CDM paradigm faces persistent small-scale challenges that have motivated alternative models for the dark sector. Sel…

astro-ph.GA2026

Bar-induced migration of Centauri away from Gaia Sausage-Enceladus

Adam M. Dillamore, Hanyuan Zhang, Vasily Belokurov

The globular cluster Cen has been suggested to have originated in the Gaia Sausage-Enceladus (GSE) merger event, possibly as its nuclear star cluster. However, the present-day…

astro-ph.SR2026

A Quadruple Excess in Wide Binary Systems: Evidence for Correlated Binary Formation

Dolev Bashi, Cathie J. Clarke, Vasily Belokurov

Understanding the multiplicity of stellar systems and the correlations between their hierarchical components provides crucial insights into star formation processes. If binary comp…

astro-ph.GA2026

The erasure of Galactic bar resonances by dark matter subhaloes

Elliot Y. Davies, Adam M. Dillamore, Vasily Belokurov +1

In the context of increasing appreciation for the coupling between the Galactic bar and the halo, we introduce a new framework using stars trapped in resonance with the bar to prob…

astro-ph.SR2026

Hide and Seek with Gaia. Detectability of Predicted Thin-Disc Metal-Rich RR Lyrae Binaries in Gaia DR3 and DR4

Giuliano Iorio, Pranav Nagarajan, Alexey Bobrick +8

RR Lyrae stars (RRLs) are classical tracers of old stellar populations, yet growing evidence suggests the presence of a metal-rich ([Fe/H]>-0.5), intermediate-age (2-7 Gyr) sub-pop…

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…