Potentially hazardous asteroids (PHAs) are objects that can have close encounters with Earth and are significantly large to cause significant regional damage in...
Mini-moons from horseshoes: A physical characterization of 2022 NX<SUB>1</SUB> with OSIRIS at the 10.4 m Gran Telescopio Canarias
Context. The near-Earth orbital space is shared by natural objects and space debris that can be temporarily captured in geocentric orbits. Short-term natural...
Misaligned spin-orbit in the XO-3 planetary system?
The transiting extrasolar planet XO-3b is remarkable, with a high mass and eccentric orbit. These unusual characteristics make it interesting to test whether...
MOBSTER: Identifying Candidate Magnetic O Stars through Rotational Modulation of TESS Photometry
O-type stars display rotational modulation of their photometric brightness due to surface features induced by fossil magnetic fields, and possibly through...
Model Selection for Spectropolarimetric Inversions
Inferring magnetic and thermodynamic information from spectropolarimetric observations relies on the assumption of a parameterized model atmosphere whose...
Model-based identification of solar coronal mass ejections using deep neural networks
Coronal mass ejections (CMEs) are a major driver of space weather and thus can have important negative technological and social impacts. To assess their...
From inversion of a time series of slit spectra, observed in a quiet region of the solar photosphere, averaged models of a granular cell have been obtained...
Moderately misaligned orbit of the warm sub-Saturn HD 332231 b
Measurements of exoplanetary orbital obliquity angles for different classes of planets are an essential tool in testing various planet formation theories...
Molar extinction coefficient of fullerenes and related hydrogenated derivatives ``fulleranes''
Fullerenes, the carbon molecules with 60 and 70 atoms, were recently detected in a series of planetary nebulae, in protoplanetary nebulae and in other...