Multi-Messenger Searches in Astrophysics
arXiv:2004.12460 · doi:10.22323/1.367.0030
Abstract
Multi-messenger astronomy has experienced an explosive development in the past few years. While not being a particularly young field, it has recently attracted a lot of attention by several major discoveries and unprecedented observation campaigns covering the entity of the electromagnetic spectrum as well as observations of cosmic rays, neutrinos, and gravitational waves. The exploration of synergies is in full steam and requires close cooperation between different instruments. Here I give an overview over the subject of multi-messenger astronomy and its virtues compared to classical "single messenger" observations, present the recent break throughs of the field, and discuss some of its organisational and technical challenges.
10 pages, 3 figures
References in corpus (12)
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector
- Neutrino emission from the direction of the blazar TXS 0506+056 prior to the IceCube-170922A alert
- Detection of the Characteristic Pion-Decay Signature in Supernova Remnants
- Observation and Characterization of a Cosmic Muon Neutrino Flux from the Northern Hemisphere using six years of IceCube data
- Acceleration of petaelectronvolt protons in the Galactic Centre
- High-energy particle acceleration in the shell of a supernova remnant
- All-sky search for time-integrated neutrino emission from astrophysical sources with 7 years of IceCube data
- How Gravitational-wave Observations Can Shape the Gamma-ray Burst Paradigm
- TeV gamma-ray observations of the binary neutron star merger GW170817 with H.E.S.S
- Introduction to multi-messenger astronomy
- Gravitational wave alert follow-up strategy in the H.E.S.S. multi-messenger framework