INTEGRAL: science highlights and future prospects
Christoph Winkler, Roland Diehl, Pietro Ubertini, and J\"orn Wilms

TL;DR
INTEGRAL has provided groundbreaking insights into high-energy astrophysics, including gamma-ray mapping, binary discoveries, and polarization detection, with future prospects for nucleosynthesis and black hole studies.
Contribution
This paper summarizes INTEGRAL's scientific achievements since 2002 and discusses future research prospects in high-energy astrophysics.
Findings
First sky map of 511 keV annihilation emission
Discovery of a new class of high-mass X-ray binaries
Detection of polarization in cosmic high-energy radiation
Abstract
ESA's hard X-ray and soft gamma-ray observatory INTEGRAL is covering the 3 keV to 10 MeV energy band, with excellent sensitivity during long and uninterrupted observations of a large field of view (~100 square degrees), with ms time resolution and keV energy resolution. It links the energy band of pointed soft X-ray missions such as XMM-Newton with that of high-energy gamma-ray space missions such as Fermi and ground based TeV observatories. Key results obtained so far include the first sky map in the light of the 511 keV annihilation emission, the discovery of a new class of high mass X-ray binaries and detection of polarization in cosmic high energy radiation. For the foreseeable future, INTEGRAL will remain the only observatory allowing the study of nucleosynthesis in our Galaxy, including the long overdue next nearby supernova, through high-resolution gamma-ray line spectroscopy.…
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