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Evolutionary models of cold and low-mass planets: Cooling curves, magnitudes, and detectability
Esther F. Linder, Christoph Mordasini, Paul Mollière +4
Future instruments like NIRCam and MIRI on JWST or METIS at the ELT will be able to image exoplanets that are too faint for current direct imaging instruments. Evolutionary models…
From cold to hot irradiated gaseous exoplanets: Toward an observation-based classification scheme
Karan Molaverdikhani, Thomas Henning, Paul Mollière
A carbon-to-oxygen ratio (C/O) of around unity is believed to act as a natural separator of water- and methane-dominated spectra when characterizing exoplanet atmospheres. In this…
Detecting isotopologues in exoplanet atmospheres using ground-based high-dispersion spectroscopy
P. Mollière, I. A. G. Snellen
Cross-correlation is a well-tested method for exoplanet characterization. A new, potentially powerful application is the measurement of atmospheric isotope ratios. In particular D/…
Discovery of a planetary-mass companion within the gap of the transition disk around PDS 70
M. Keppler, M. Benisty, A. Müller +123
Young circumstellar disks are of prime interest to understand the physical and chemical conditions under which planet formation takes place. Only very few detections of planet cand…
Orbital and atmospheric characterization of the planet within the gap of the PDS 70 transition disk
A. Müller, M. Keppler, Th. Henning +43
Aims: We aim to characterize the orbital and atmospheric properties of PDS 70 b, which was first identified on May 2015 in the course of the SHINE survey with SPHERE, the extreme a…