activity
20172024
most citedAtomic iron and titanium in the atmosphere of the exoplanet KELT-9b

252 citations · 2.9k across the 46 of their papers we have counts for

collaborators
Showing 2019Show all

5 papers · 1 filter

astro-ph.EP2019★ 75 cited

Wind of Change: retrieving exoplanet atmospheric winds from high-resolution spectroscopy

J. V. Seidel, D. Ehrenreich, L. Pino +5

Context. The atmosphere of exoplanets has been studied extensively in recent years, using numerical models to retrieve chemical composition, dynamical circulation or temperature fr…

astro-ph.EP2019★ 32 cited

The potassium absorption on HD189733b and HD209458b

Engin Keles, Matthias Mallonn, Carolina von Essen +9

In this work, we investigate the potassium excess absorption around 7699A of the exoplanets HD189733b and HD209458b. For this purpose, we used high spectral resolution transit obse…

astro-ph.EP2019★ 81 cited

Optical phase curve of the ultra-hot Jupiter WASP-121b

V. Bourrier, D. Kitzmann, T. Kuntzer +28

We present the analysis of TESS optical photometry of WASP-121b, which reveal the phase curve of this transiting ultra-hot Jupiter. Its hotspot is located at the substellar point,…

astro-ph.EP2019★ 231 cited

A spectral survey of an ultra-hot Jupiter: Detection of metals in the transmission spectrum of KELT-9 b

H. J. Hoeijmakers, D. Ehrenreich, D. Kitzmann +16

Context: KELT-9 b exemplifies a newly emerging class of short-period gaseous exoplanets that tend to orbit hot, early type stars - termed ultra-hot Jupiters. The severe stellar irr…

astro-ph.EP2019★ 130 cited

Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS) - II. A broadened sodium feature on the ultra-hot giant WASP-76b

J. V. Seidel, D. Ehrenreich, A. Wyttenbach +18

High-resolution optical spectroscopy is a powerful tool to characterise exoplanetary atmospheres from the ground. The sodium D lines, with their large cross sections, are especiall…