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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5 papers · 1 filter

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.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.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.SR2025

Revealing the ages of metal-rich RR Lyrae via kinematic label transfer

HanYuan Zhang, Giuliano Iorio, Vasily Belokurov +3

RR Lyrae stars have long been considered reliable tracers of old, metal-poor populations, primarily due to their prevalence in globular clusters and the Galactic halo. However, the…

astro-ph.SR2024★ 15 cited

Predicting metallicities and carbon abundances from Gaia XP spectra for (carbon-enhanced) metal-poor stars

Anke Ardern-Arentsen, Sarah G. Kane, Vasily Belokurov +4

Carbon-rich (C-rich) stars can be found at all metallicities and evolutionary stages. They are often the result of mass-transfer from a companion, but some of the most metal-poor C…