We present analysis of the atmospheres of 70 gaseous extrasolar planets via transit
spectroscopy with Hubble's Wide Field Camera 3 (WFC3). For over half of these, we …

The ExoClock project is an inclusive, integrated, and interactive platform that was developed
to monitor the ephemerides of the Ariel targets to increase the mission efficiency. The project …

The number of exoplanets discovered already exceeds 5000 and continues to increase
daily. The characterization of exoplanets will be the main goal of future space missions. The …

We analyze a large number of citizen science data and identify eight hot Jupiter systems that
show evidence for deviations from a constant orbital period: HAT-P-19 b, HAT-P-32 b, TrES …

We present the discovery and characterization of six short-period, transiting giant planets
from NASA's Transiting Exoplanet Survey Satellite (TESS)--TOI-1811 (TIC 376524552), TOI …

Accurate physical parameters of exoplanet systems are essential for further exploration of
planetary internal structure, atmospheres, and formation history. We aim to use …

We present 14 simultaneous Chandra X‐ray Observatory (CXO)‐Hubble Space Telescope
(HST) observations of Jupiter's Northern X‐ray and ultraviolet (UV) aurorae from 2016 to …

Thanks to their short orbital periods and hot extended atmospheres, hot Jupiters are ideal
candidates for atmosphere studies with high-resolution spectroscopy. New stable …

Hot Jupiters should initially form at considerable distances from host stars and subsequently
migrate towards inner regions, supported directly by transit timing variation (TTV). We report …

Core-collapse supernovae (CCSNe) are capable of producing large quantities of dust, with
strong evidence that ejecta dust masses can grow significantly over extended periods of …