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Astronomy and astrophysics are the study of objects and phenomena that are found beyond our solar system. This combines theoretical simulations and observation with both terrestrial and space-craft-borne instruments of the electromagnetic radiation and high-energy particles emitted by celestial bodies.
Phase-curve observations of the ‘hot Jupiter’ exoplanet WASP-43b, made at mid-infrared wavelengths using JWST, provide evidence that fast winds limit the formation of methane on the cooler, cloudy nightside of the planet.
Observations have revealed a galaxy that stopped forming stars earlier than expected. This discovery offers clues about when the first galaxies emerged and sheds light on how stars formed when the Universe was in its infancy.
Computer simulations based on the prevailing cosmological model, ΛCDM, reproduce many observed properties of our Universe. But a study of coherent satellite motions in galaxy clusters yields discrepancies that challenge the definition of ‘today’.
Decametre radio observations are challenging due to the presence of the ionosphere. Here Groeneveld et al. present a strategy to correct for the ionosphere that allows them to make sharp decametre radio images from the ground with the LOFAR telescope.
Phase-resolved mid-infrared observations from JWST of the hot gas giant WASP-43b detect a day–night difference of 659 ± 19 K. Comparison with climate models shows that the observations are compatible with cloudy skies, at least on the nightside, and the lack of methane detection suggests the presence of disequilibrium chemistry.
Energetic neutrino beams from symmetric muon and anti-muon decays are used to study long-baseline neutrino oscillation, and constrain the Charge-Parity (CP) violation phase in the three-flavour neutrino mixing. Here, the authors provide results based on neutrino oscillation simulations to show that more than five standard deviation sensitivity on CP violation can be obtained from 5-10 years of data taken with the help of DUNE-like detectors.
We report observations of GRB 231115A, positionally coincident with the starburst galaxy M82, that unambiguously qualify this burst as a giant flare from a magnetar, which is a rare explosive event releasing gamma rays.
A three-dimensional reconstruction of a bright flare orbiting the black hole Sagittarius A* is computationally recovered from ALMA light curve data by constraining a neural network with a gravitational model of black holes.
The first set of results from a pioneering cosmic-mapping project hints that the repulsive force known as dark energy has changed over 11 billion years, which would alter ideas about how the Universe has evolved and what its future will be.
Phase-curve observations of the ‘hot Jupiter’ exoplanet WASP-43b, made at mid-infrared wavelengths using JWST, provide evidence that fast winds limit the formation of methane on the cooler, cloudy nightside of the planet.