The application of machine learning in solar physics has the potential to greatly enhance our understanding of the complex processes that take place in the...
Machine learning initialization to accelerate Stokes profile inversions
Context. At present, an exponential growth in scientific data from current and upcoming solar observatories is expected. Most of the data consist of high...
Machine-learning approaches to exoplanet transit detection and candidate validation in wide-field ground-based surveys
Since the start of the Wide-angle Search for Planets (WASP) program, more than 160 transiting exoplanets have been discovered in the WASP data. In the past...
Macromolecular organic matter in samples of the asteroid (162173) Ryugu
Samples of the carbonaceous asteroid (162173) Ryugu were collected and brought to Earth by the Hayabusa2 spacecraft. We investigated the macromolecular organic...
Made-to-measure models of the Galactic box/peanut bulge: stellar and total mass in the bulge region
We construct dynamical models of the Milky Way's box/peanut (B/P) bulge, using the recently measured 3D density of red clump giants (RCGs) as well as kinematic...
MAG Waves in Sunspots Umbrae: Slow Waves Leaking to the Corona
The linear oscillations of a stratified atmosphere embedded in a uniform vertical magnetic field are studied here. We use a simple theoretical model, formed by...
MAGIC and Fermi-LAT gamma-ray results on unassociated HAWC sources
The HAWC Collaboration released the 2HWC catalogue of TeV sources, in which 19 show no association with any known high-energy (HE; E ≳ 10 GeV) or very-high...
Magic Constraints on γ-ray Emission from Cygnus X-3
Cygnus X-3 is a microquasar consisting of an accreting compact object orbiting around a Wolf-Rayet star. It has been detected at radio frequencies and up to...
Gamma-ray bursts (GRBs) are explosive transient events occurring at cosmological distances, releasing a large amount of energy as electromagnetic radiation over...