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- Helmholtz-Zentrum Berlin für Materialien und EnergieDE144 papers
- Centre National de la Recherche ScientifiqueFR132 papers
- Technische Universität BerlinDE127 papers
- Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR)DE97 papers
- University of CambridgeGB78 papers
- Sorbonne UniversitéFR77 papers
- Leiden UniversityNL71 papers
- University of GenevaCH70 papers
- Chalmers University of TechnologySE68 papers
- Austrian Academy of SciencesAT67 papers
- Stockholm UniversitySE67 papers
- University of WarwickGB67 papers
6 papers · 2 filters
Giant Outer Transiting Exoplanet Mass (GOTEM) Survey.VII. TOI-6041: a multi-planet system including a warm Neptune exhibiting strong TTVs
N. Heidari, A. Alnajjarine, H. P. Osborn +101
We present the characterization of the TOI-6041 system, a bright () G7-type star hosting at least two planets. The inner planet, TOI-6041b, is a warm Neptune wit…
Improved characterization of the TOI-2141 system: a dense sub-Neptune with non-transiting inner and outer companions
R. Luque, K. W. F. Lam, J. Cabrera +87
We aim to refine the fundamental parameters of the TOI-2141 planetary system, which includes a transiting sub-Neptune orbiting a Sun-like star in a relatively long orbit of 18.26 d…
The influence of interior structure and thermal state on impact melt generation upon large impacts onto terrestrial planets
Lukas Manske, Thomas Ruedas, Ana-Catalina Plesa +4
We investigate the melt production of planetary impacts as a function of planet size (=0.1-1.5), impactor size (=1-1000 km), and core size ratio ($R_\mathrm{…
Dark skies of the slightly eccentric WASP-18 b from its optical-to-infrared dayside emission
A. Deline, P. E. Cubillos, L. Carone +86
We performed a joint analysis of phase-curve observations of the ultra-hot Jupiter WASP-18 b from the visible to the mid-infrared, using data from CHEOPS, TESS and Spitzer. We aim…
The PLATO field selection process. II. Characterization of LOPS2, the first long-pointing field
V. Nascimbeni, G. Piotto, J. Cabrera +26
PLAnetary Transits and Oscillations of stars (PLATO) is an ESA M-class mission to be launched by the end of 2026 to discover and characterize transiting planets around bright and n…
Characterizing WASP-43b's interior structure: unveiling tidal decay and apsidal motion
Lia Marta Bernabò, Szilárd Csizmadia, Alexis M. S. Smith +8
Context. Recent developments in exoplanetary research highlight the importance of Love numbers in understanding their internal dynamics, formation, migration history and their pote…