activity
20122026
most citedFundamental Properties of Stars using Asteroseismology from Kepler & CoRoT and Interferometry from the CHARA Array

260 citations · 314 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2026

Detailed Abundance Determination of Metal-Poor Stars with X-Shooter II. - Chemically Disentangling the Halo, Disk and GSE

Benjamin D. C. Lowe, Luca Casagrande, Thomas Nordlander +2

We present a detailed chemical analysis of seven extremely metal-poor (EMP) star candidates observed with X-Shooter, combining them with 16 EMP candidates from Paper I. We measured…

astro-ph.SR2026★ 1 cited

High-fidelity stellar extinction with Gaia and APOGEE -- I. The method and a new extinction curve

Jie Yu, Luca Casagrande, John A. Taylor +9

The scarcity of high-fidelity extinction measurements remains a bottleneck in deriving accurate stellar properties from Gaia parallaxes. In this work, we aim to derive precision ex…

astro-ph.EP2025

C3PO IV: co-natal stars depleted in refractories are magnetically more active -- possible imprints of planets

Jie Yu, Yuan-Sen Ting, Luca Casagrande +14

Chemical abundance anomalies in twin stars have recently been considered tell-tale signs of interactions between stars and planets. While such signals are prevalent, their nature r…

astro-ph.GA2025★ 3 cited

The Rise of the Milky Way Disk through EMP Stars

B. Lowe, T. Nordlander, L. Casagrande +6

We present a chemo-dynamical study conducted with 2dFAAOmega of Gaia DR3 non-variable candidate metal-poor stars that lie in the direction of the Galactic plane. Our…

astro-ph.GA2024

Survey of extended Main Sequence Turn-offs in Galactic Open Clusters: Stellar rotations from Gaia RVS spectra

Giacomo Cordoni, Luca Casagrande, Jie Yu +6

The origin of extended main-sequence turn-offs (eMSTO) in star clusters younger than 2 Gyr still challenges our current understanding of stellar evolution. Exploiting data from Gai…

astro-ph.GA2024★ 20 cited

The GALAH survey: Tracing the Milky Way's formation and evolution through RR Lyrae stars

Valentina D'Orazi, Nicholas Storm, Andrew R. Casey +39

Stellar mergers and accretion events have been crucial in shaping the evolution of the Milky Way (MW). These events have been dynamically identified and chemically characterised us…

astro-ph.SR2024

New Evidence of Binarity in Young α-Rich Turn-off and Subgiant Stars: Fast Rotation and Strong Magnetic Activity

Jie Yu, Luca Casagrande, Ioana Ciucă +3

Young α-rich (YAR) stars within the old Galactic thick disk exhibit a dual characteristic of relative youth determined with asteroseismology and abundance enhancement in α elements…

astro-ph.SR2024★ 10 cited

Cool and Data-Driven: An Exploration of Optical Cool Dwarf Chemistry with Both Data-Driven and Physical Models

Adam D. Rains, Thomas Nordlander, Stephanie Monty +6

Detailed chemical studies of F/G/K -- or Solar-type -- stars have long been routine in stellar astrophysics, enabling studies in both Galactic chemodynamics, and exoplanet demograp…

astro-ph.SR2018★ 12 cited

On the AGB stars of M 4: A robust disagreement between spectroscopic observations and theory

B. T. MacLean, S. W. Campbell, A. M. Amarsi +7

Several recent spectroscopic investigations have presented conflicting results on the existence of Na-rich asymptotic giant branch (AGB) stars in the Galactic globular cluster M4 (…

astro-ph.SR2017★ 8 cited

AGB subpopulations in the nearby globular cluster NGC 6397

B. T. MacLean, S. W. Campbell, G. M. De Silva +5

It has been well established that Galactic Globular clusters (GCs) harbour more than one stellar population, distinguishable by the anti-correlations of light element abundances (C…

astro-ph.SR2012★ 260 cited

Fundamental Properties of Stars using Asteroseismology from Kepler & CoRoT and Interferometry from the CHARA Array

D. Huber, M. J. Ireland, T. R. Bedding +37

We present results of a long-baseline interferometry campaign using the PAVO beam combiner at the CHARA Array to measure the angular sizes of five main-sequence stars, one subgiant…