activity
20212025
most citedThe Gaia-ESO Public Spectroscopic Survey: Implementation, data products, open cluster survey, science, and legacy

188 citations · 523 across the 20 of their papers we have counts for

collaborators

20 papers

astro-ph.SR2025★ 1 cited

Glitch analysis and asteroseismic modelling of subgiant Herculis: confirming and interpreting the peak as the helium glitch

Advik Gupta, Kuldeep Verma, Hans Kjeldsen +7

The measurements of pressure-mode and mixed-mode oscillation frequencies in subgiant stars offer a unique opportunity to probe their internal structures -- from the surface to the…

astro-ph.SR2025★ 5 cited

Pushing the boundaries of asteroseismic individual frequency modelling: unveiling two evolved very-low metallicity red giants

Jens R. Larsen, Jakob L. Rørsted, Victor Aguirre Børsen-Koch +21

Metal-poor stars are key to understanding the first stellar generation in the Galaxy. Asteroseismic characterisation of red giants has traditionally relied on global seismic parame…

astro-ph.EP2024

A link between rocky exoplanet composition and stellar age

Angharad Weeks, Vincent Van Eylen, Daniel Huber +7

Interior compositions are key for our understanding of Earth-like exoplanets. The composition of the core can influence the presence of a magnetic dynamo and the strength of gravit…

astro-ph.SR2024

Stellar Models are Reliable at Low Metallicity: An Asteroseismic Age for the Ancient Very Metal-Poor Star KIC 8144907

Daniel Huber, Ditte Slumstrup, Marc Hon +15

Very metal-poor stars ([Fe/H]<-2) are important laboratories for testing stellar models and reconstructing the formation history of our galaxy. Asteroseismology is a powerful tool…

astro-ph.IM2024★ 13 cited

The PLATO Mission

Heike Rauer, Conny Aerts, Juan Cabrera +842

PLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large numb…

astro-ph.SR2024★ 12 cited

The K2 Asteroseismic KEYSTONE sample of Dwarf and Subgiant Solar-Like Oscillators. I: Data and Asteroseismic parameters

Mikkel N. Lund, Sarbani Basu, Allyson Bieryla +19

The KEYSTONE project aims to enhance our understanding of solar-like oscillators by delivering a catalogue of global asteroseismic parameters ( and ) for 173 s…

astro-ph.SR2024★ 16 cited

An extended and refined grid of 3D STAGGER model atmospheres. Processed snapshots for stellar spectroscopy

Luisa F. Rodríguez Díaz, Cis Lagae, Anish M. Amarsi +6

Context: Traditional one-dimensional (1D) hydrostatic model atmospheres introduce systematic modelling errors into spectroscopic analyses of FGK-type stars. Aims: We present an upd…

astro-ph.GA2024★ 8 cited

Exploring the dependence of chemical traits on metallicity: chemical trends for red giant stars with asteroseismic ages

S. Vitali, D. Slumstrup, P. Jofré +5

Given the massive spectroscopic surveys and the Gaia mission, the Milky Way has turned into a unique laboratory to be explored using abundance ratios that show a strong dependency…

astro-ph.SR2023★ 18 cited

3D Stagger model atmospheres with FreeEOS I. Exploring the impact of microphysics on the Sun

Yixiao Zhou, Anish M. Amarsi, Victor Aguirre Børsen-Koch +3

Three-dimensional radiation-hydrodynamics (3D RHD) simulations of stellar surface convection provide valuable insights into many problems in solar and stellar physics. However, alm…

astro-ph.GA2023★ 14 cited

A Unified Exploration of the Chronology of the Galaxy

Amalie Stokholm, Víctor Aguirre Børsen-Koch, Dennis Stello +2

The Milky Way has distinct structural stellar components linked to its formation and subsequent evolution, but disentangling them is nontrivial. With the recent availability of hig…

astro-ph.SR2023

Did Kepler-444 have a long-lived convective core?

Mark Lykke Winther, Víctor Aguirre Børsen-Koch, Jakob Lysgaard Rørsted +2

With the greater power to infer the state of stellar interiors provided by asteroseismology, it has become possible to study the survival of initially convective cores within stars…

astro-ph.SR2022★ 133 cited

The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products

G. Gilmore, S. Randich, C. C. Worley +165

The Gaia-ESO Public Spectroscopic Survey is an ambitious project designed to obtain astrophysical parameters and elemental abundances for 100,000 stars, including large representat…

astro-ph.SR2022

Advanced asteroseismic modelling: breaking the degeneracy between stellar mass and initial helium abundance

Kuldeep Verma, Jakob L. Rørsted, Aldo M. Serenelli +3

Current stellar model predictions of adiabatic oscillation frequencies differ significantly from the corresponding observed frequencies due to the non-adiabatic and poorly understo…

astro-ph.GA2022★ 188 cited

The Gaia-ESO Public Spectroscopic Survey: Implementation, data products, open cluster survey, science, and legacy

S. Randich, G. Gilmore, L. Magrini +161

In the last 15 years different ground-based spectroscopic surveys have been started (and completed) with the general aim of delivering stellar parameters and elemental abundances f…

astro-ph.SR2022

Scaling relations of convective granulation noise across the HR diagram from 3D stellar atmosphere models

Luisa Fernanda Rodríguez Díaz, Lionel Bigot, Víctor Aguirre Børsen-Koch +5

High-precision photometric data from space missions have improved our understanding of stellar granulation. These observations have shown with precision the stochastic brightness f…

astro-ph.GA2022★ 16 cited

Disc dichotomy signature in the vertical distribution of [Mg/Fe] and the delayed gas infall scenario

E. Spitoni, V. Aguirre Børsen-Koch, K. Verma +1

The analysis of the APOGEE data suggests the existence of a clear distinction between two sequences of disc stars in the [/Fe] vs. [Fe/H] abundance ratio space. We aim to test i…

astro-ph.SR2021★ 10 cited

Chemo-dynamics and asteroseismic ages of seven metal-poor red giants from the Kepler field

Arthur Alencastro Puls, Luca Casagrande, Stephanie Monty +5

In this work we combine information from solar-like oscillations, high-resolution spectroscopy and Gaia astrometry to derive stellar ages, chemical abundances and kinematics for a…

astro-ph.GA2021★ 27 cited

Age Determination of Galaxy Merger Remnant Stars using Asteroseismology

Camilla C. Borre, Víctor Aguirre Børsen-Koch, Amina Helmi +12

The Milky Way was shaped by the mergers with several galaxies in the past. We search for remnant stars that were born in these foreign galaxies and assess their ages in an effort t…

astro-ph.SR2021

PLATO Hare-and-Hounds exercise: Asteroseismic model fitting of main-sequence solar-like pulsators

M. S. Cunha, I. W. Roxburgh, V. Aguirre Børsen-Koch +19

Asteroseismology is a powerful tool to infer fundamental stellar properties. The use of these asteroseismic-inferred properties in a growing number of astrophysical contexts makes…

astro-ph.SR2021★ 62 cited

The BAyesian STellar Algorithm (BASTA): a fitting tool for stellar studies, asteroseismology, exoplanets, and Galactic archaeology

V. Aguirre Børsen-Koch, J. L. Rørsted, A. B. Justesen +16

We introduce the public version of the BAyesian STellar Algorithm (BASTA), an open-source code written in {\tt Python} to determine stellar properties based on a set of astrophysic…