newASTROGAM -- The New MeV to GeV Gamma-ray Observatory
D. Berge (1, 2), M. N. Mazziotta (3), M. Tavani (4), V. Tatischeff (5), U. Oberlack (6) (for the newASTROGAM proposal team, (1) Deutsches Elektronen-Synchrotron DESY, Germany, (2) Humboldt-University of Berlin, Institute of Physics, Germany, (3) INFN, Bari, Italy

TL;DR
newASTROGAM is a proposed space mission designed to explore the under-studied MeV gamma-ray range with advanced detectors, aiming to address key astrophysical questions and detect multi-messenger sources from space.
Contribution
It introduces a novel gamma-ray observatory concept with unprecedented sensitivity, resolution, and broad energy coverage from keV to GeV energies.
Findings
Design of a Silicon tracker and crystal calorimeter payload
Potential to detect and study key astrophysical sources in the MeV to GeV range
Capability to constrain dark matter and study compact objects
Abstract
newASTROGAM is a breakthrough mission concept for the study of the non-thermal Universe from space with gamma rays in the energy range from 15 keV to 3 GeV. It is based on advanced space-proven detector technologies, which will achieve unprecedented sensitivity, angular and energy resolution combined with polarimetric capability. Since the MeV gamma-ray energy range is the most under-explored electromagnetic window to the Universe, a mission in this energy range can for the first time sensitively address fundamental astrophysics questions connected to the physics of compact objects and merger events, jets and their environments, supernovae and the origin of the elements, potentially constrain the nature of dark matter and many more science objectives. The mission will detect and follow-up many of the key sources of multi-messenger astronomy in the 2040s. newASTROGAM provides an…
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