activity
20182022
most citedDeciphering the atmosphere of HAT-P-12b: solving discrepant results

63 citations · 286 across the 9 of their papers we have counts for

collaborators

9 papers

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.EP2022★ 3 cited

On the parameter refinement of inflated exoplanets with large radius uncertainty based on TESS observations

Xanthippi Alexoudi

We revisited ten known exoplanetary systems using publicly available data provided by the Transiting Exoplanet Survey Satellite (TESS). The sample presented in this work consists o…

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…

astro-ph.EP2020★ 16 cited

Role of the impact parameter in exoplanet transmission spectroscopy

X. Alexoudi, M. Mallonn, E. Keles +3

Transmission spectroscopy is a promising tool for the atmospheric characterization of transiting exoplanets. Because the planetary signal is faint, discrepancies have been reported…

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★ 41 cited

Low albedos of hot to ultra-hot Jupiters in the optical to near-infrared transition regime

M. Mallonn, J. Köhler, X. Alexoudi +4

The depth of a secondary eclipse contains information of both the thermally emitted light component of a hot Jupiter and the reflected light component. If the dayside atmosphere of…

astro-ph.EP2019★ 33 cited

Ephemeris refinement of 21 Hot Jupiter exoplanets with high timing uncertainties

M. Mallonn, C. von Essen, E. Herrero +32

Transit events of extrasolar planets offer a wealth of information for planetary characterization. However, for many known targets, the uncertainty of their predicted transit windo…

astro-ph.EP2018★ 63 cited

Deciphering the atmosphere of HAT-P-12b: solving discrepant results

X. Alexoudi, M. Mallonn, C. von Essen +9

Two independent investigations of the atmosphere of the hot Jupiter HAT-P-12b by two different groups resulted in discrepant solutions. Using broad-band photometry from the ground,…

astro-ph.SR2018★ 54 cited

GJ1214: Rotation period, starspots, and uncertainty on the optical slope of the transmission spectrum

M. Mallonn, E. Herrero, I. G. Juvan +6

Brightness inhomogeneities in the stellar photosphere (dark spots or bright regions) affect the measurements of the planetary transmission spectrum. To investigate the star spots o…