activity
20022024
most citedThe PLATO 2.0 Mission

1.3k citations · 8.7k across the 61 of their papers we have counts for

collaborators

61 papers

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.SR2023★ 9 cited

Does the scaling relation depend on metallicity? Insights from 3D convection simulations

Yixiao Zhou, Jørgen Christensen-Dalsgaard, Martin Asplund +4

Solar-like oscillations have been detected in thousands of stars thanks to modern space missions. These oscillations have been used to measure stellar masses and ages, which have b…

astro-ph.GA2021★ 11 cited

Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. VIII. Carbon and oxygen

T. Bensby, A. Gould, M. Asplund +6

CONTEXT: [ABRIDGED]. For the Milky Way bulge, there are currently essentially no measurements of carbon in un-evolved stars, hampering our abilities to properly compare Galactic ch…

astro-ph.IM2020★ 186 cited

Atomic data for the Gaia-ESO Survey

Ulrike Heiter, Karin Lind, Maria Bergemann +27

We describe the atomic and molecular data that were used for the abundance analyses of FGK-type stars carried out within the Gaia-ESO Survey. We present an unprecedented effort to…

astro-ph.GA2020★ 117 cited

The GALAH survey: tracing the Galactic disk with Open Clusters

Lorenzo Spina, Yuan-Sen Ting, Gayandhi M. De Silva +28

Open clusters are unique tracers of the history of our own Galaxy's disk. According to our membership analysis based on \textit{Gaia} astrometry, out of the 226 potential clusters…

astro-ph.SR2020★ 44 cited

Detailed chemical compositions of planet hosting stars: I. Exploration of possible planet signatures

F. Liu, D. Yong, M. Asplund +5

We present a line-by-line differential analysis of a sample of 16 planet hosting stars and 68 comparison stars using high resolution, high signal-to-noise ratio spectra gathered us…