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

collaborators

62 papers

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…

astro-ph.IM2025

Galaxies as stochastic systems: why the next breakthrough in galaxy evolution requires one hundred million spectra

Sandro Tacchella, Vasily Belokurov, Harry T. J. Bevins +4

Each galaxy is observed only once along its life, making galaxy evolution fundamentally an inverse statistical problem: time-dependent physics must be inferred from ensembles of si…

astro-ph.GA2025

Orbital migration and heating history of the Galactic disc: a transition between the bimodal discs

HanYuan Zhang, Vasily Belokurov, Jason L. Sanders +7

Stellar orbits in the Galactic disc evolve from their birth to the current shape through both radial migration and dynamical heating. The history of their secular evolution is impr…

astro-ph.GA2025

Enhanced rates of stellar radial migration in gas-rich discs at high redshift

HanYuan Zhang, Thor Tepper-García, Vasily Belokurov +6

Radial migration and dynamical heating redistribute stars within galactic discs and thereby modify the chemo-kinematic structure of their host galaxies. Usually, these secular proc…

astro-ph.GA2025★ 5 cited

STRRINGS: STReams in Residual Images of Nearby GalaxieS

E. Sola, D. Chemaly, V. Belokurov +11

Tidal features from galaxy mergers, particularly stellar streams, offer valuable insights into galaxy assembly and dark matter halo properties. This paper aims to identify a large…

astro-ph.GA2025★ 1 cited

On the connection between nitrogen-enhanced field stars and the Galactic globular clusters

Sarah G. Kane, Vasily Belokurov, Stephanie Monty +6

As sites of some of the most efficient star formation in the Universe, globular clusters (GCs) have long been hypothesized to be the building blocks of young galaxies. Within the M…

astro-ph.GA2025★ 2 cited

JADES: the chemical enrichment pattern of distant galaxies -- enhancement, silicon depletion, and iron enhancement

Yuki Isobe, Roberto Maiolino, Xihan Ji +26

We present gas-phase abundances of carbon (C), -elements (O, Ne, Si, and Ar) and iron (Fe) obtained from stacked spectra of high- star-forming galaxies with the deep Near Inf…

astro-ph.GA2025

Lord of LRDs: Insights into a "Little Red Dot" with a low-ionization spectrum at z = 0.1

Xihan Ji, Francesco D'Eugenio, Ignas Juodžbalis +14

Recent observations by the James Webb Space Telescope (JWST) have revealed a puzzling population of optically red and compact galaxies with peculiar "V"-shaped spectra at high reds…

astro-ph.GA2025★ 5 cited

The THESAN-ZOOM project: Mystery N/O more -- uncovering the origin of peculiar chemical abundances and a not-so-fundamental metallicity relation at

William McClymont, Sandro Tacchella, Aaron Smith +15

We present an analysis of metallicities and chemical abundances at in the THESAN-ZOOM simulations. We find that smoothly curved gas-phase and stellar mass-metallicity rela…

astro-ph.SR2025★ 4 cited

Fewer Companions in the Crowd: The Low Close Binary Fraction in Globular Clusters from Gaia RVS

Dolev Bashi, Vasily Belokurov

In dense environments like globular clusters (GCs), dynamical interactions can disrupt or harden close binaries, nonetheless, detailed comparisons with field binary fractions remai…

astro-ph.GA2025★ 8 cited

The completeness of the open cluster census towards the Galactic anticentre

Emily L. Hunt, Tristan Cantat-Gaudin, Friedrich Anders +9

Open clusters have long been used as tracers of Galactic structure. However, without a selection function to describe the completeness of the cluster census, it is difficult to qua…