activity
20082024
most citedTransiting exoplanets from the CoRoT space mission I - CoRoT-Exo-1b: a low-density short-period planet around a G0V star

221 citations · 1.8k across the 33 of their papers we have counts for

collaborators

33 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.SR2024★ 1 cited

Understanding the effects of spacecraft trajectories through solar coronal mass ejection flux ropes using 3DCOREweb

Hannah Theresa Rüdisser, Andreas Jeffrey Weiss, Justin Le Louëdec +4

This study investigates the impact of spacecraft positioning and trajectory on in situ signatures of coronal mass ejections (CMEs). Employing the 3DCORE model, a 3D flux rope model…

astro-ph.EP2024★ 15 cited

CAI formation in the early Solar System

P. Woitke, J. Drażkowska, H. Lammer +2

Ca-Al-rich inclusions (CAIs) are the oldest dated solid materials in the solar system, found as light-coloured crystalline ingredients in meteorites. Their formation time is common…

astro-ph.EP2023★ 1 cited

On the required mass for exoplanetary radio emission

Jean-Mathias Grießmeier, N. V. Erkaev, C. Weber +3

The detection of radio emission from an exoplanet would constitute the best way to determine its magnetic field. Indeed, the presence of a planetary magnetic field is a necessary c…

astro-ph.SR2020★ 48 cited

A census of Coronal Mass Ejections on solar-like stars

M. Leitzinger, P. Odert, R. Greimel +8

Coronal Mass Ejections (CMEs) may have major importance for planetary and stellar evolution. Stellar CME parameters, such as mass and velocity, have yet not been determined statist…

astro-ph.EP2020★ 22 cited

Three-dimensional modelling of absorption by various species for hot Jupiter HD 209458b

I F Shaikhislamov, M L Khodachenko, H Lammer +3

The absorption of stellar radiation observed by the HD209458b in resonant lines of OI and CII has not yet been satisfactorily modeled. In our previous 2D simulations we have shown…