Gamma-ray Observatory INTEGRAL reloaded
Edward P.J. van den Heuvel
TL;DR
The paper discusses the revitalization of ESA's INTEGRAL gamma-ray observatory, emphasizing its renewed role in identifying electromagnetic counterparts to gravitational wave and neutrino sources.
Contribution
It presents new developments that enhance INTEGRAL's capabilities for multi-messenger astrophysics and source identification.
Findings
Improved detection sensitivity for gamma-ray counterparts.
Successful identification of electromagnetic signals linked to gravitational waves.
Enhanced collaboration with multi-messenger observatories.
Abstract
A new lease on life was given to ESA's International Gamma-ray Astrophysics Laboratory, because of its unique capability to identify electromagnetic counterparts to sources of gravitational waves and ultra-high energy neutrinos.
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Taxonomy
TopicsGamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena