Ponente
Descripción
Space-based gamma-ray observatories provide continuous, all-sky coverage from a few hundred keV to hundreds of GeV, bridging the hard X-ray and very-high-energy domains accessible from the ground. Instruments such as Swift-BAT, INTEGRAL, Fermi-GBM, and Fermi-LAT, among others, have enabled precision studies of non-thermal processes in astrophysical sources, cosmological measurements through the extragalactic background light and large-scale structure correlations, and time-domain discoveries of transient phenomena. In this talk, I will review key achievements and recent highlights of gamma-ray astrophysics from space, and discuss upcoming missions designed to close the MeV sensitivity gap and expand discovery space in polarization, timing, and broadband spectroscopy—advancing our understanding of the high-energy Universe.
