activity
20072024
most citedPEPSI: The high-resolution echelle spectrograph and polarimeter for the Large Binocular Telescope

170 citations · 1.2k across the 47 of their papers we have counts for

collaborators

47 papers

astro-ph.EP2024

The PEPSI Exoplanet Transit Survey (PETS). V: New Na D transmission spectra indicate a quieter atmosphere on HD 189733b

E. Keles, S. Czesla, K. Poppenhaeger +23

Absorption lines from exoplanet atmospheres observed in transmission allow us to study atmospheric characteristics such as winds. We present a new high-resolution transit time-seri…

astro-ph.SR2023★ 11 cited

Zeeman Doppler Imaging of ksi Boo A and B

K. G. Strassmeier, T. A. Carroll, I. V. Ilyin

We present a magnetic-field surface map for both stellar components of the young visual binary ksi Boo AB (A: G8V, B: K5V). Employed are high resolution Stokes-V spectra obtained w…

astro-ph.SR2023★ 7 cited

VPNEP: Detailed characterization of TESS targets around the Northern Ecliptic Pole

K. G. Strassmeier, M. Weber, D. Gruner +13

We embarked on a high-resolution optical spectroscopic survey of bright Transiting Exoplanet Survey Satellite (TESS) stars around the Northern Ecliptic Pole (NEP), dubbed the Vatic…

astro-ph.EP2022★ 34 cited

The PEPSI Exoplanet Transit Survey (PETS) I: Investigating the presence of a silicate atmosphere on the super-Earth 55 Cnc e

Engin Keles, Matthias Mallonn, Daniel Kitzmann +26

The study of exoplanets and especially their atmospheres can reveal key insights on their evolution by identifying specific atmospheric species. For such atmospheric investigations…

astro-ph.SR2021★ 14 cited

A confined dynamo: magnetic activity of the K-dwarf component in the pre-cataclysmic binary system V471 Tauri

Zs. Kővári, L. Kriskovics, K. Oláh +6

We scrutinize the red dwarf component in the eclipsing binary system V471 Tau in order to unravel relations between different activity layers from the stellar surface through the c…

astro-ph.EP2020★ 10 cited

Probing the atmosphere of HD189733b with the Na I and K I lines

E. Keles, D. Kitzmann, M. Mallonn +12

High spectral resolution transmission spectroscopy is a powerful tool to characterize exoplanet atmospheres. Especially for hot Jupiters, this technique is highly relevant, due to…