Strategies for the Follow-up of Gravitational Wave Transients with the Cherenkov Telescope Array

The observation of the electromagnetic counterpart of gravitational-wave (GW) transient GW170817 demonstrated the potential in extracting astrophysical information from multimessenger discoveries. The forthcoming deployment of the first telescopes of the Cherenkov Telescope Array (CTA) observatory w...

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Hauptverfasser: Bartos, Imre, Tristano Di Girolamo, Gair, Jonathan R, Hendry, Martin, Heng, Ik Siong, Humensky, T Brian, Marka, Szabolcs, Marka, Zsuzsa, Messenger, Chris, Mukherjee, Reshmi, Nieto, Daniel, O'Brien, Paul, Santander, Marcos
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container_title arXiv.org
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creator Bartos, Imre
Tristano Di Girolamo
Gair, Jonathan R
Hendry, Martin
Heng, Ik Siong
Humensky, T Brian
Marka, Szabolcs
Marka, Zsuzsa
Messenger, Chris
Mukherjee, Reshmi
Nieto, Daniel
O'Brien, Paul
Santander, Marcos
description The observation of the electromagnetic counterpart of gravitational-wave (GW) transient GW170817 demonstrated the potential in extracting astrophysical information from multimessenger discoveries. The forthcoming deployment of the first telescopes of the Cherenkov Telescope Array (CTA) observatory will coincide with Advanced LIGO/Virgo's next observing run, O3, enabling the monitoring of gamma-ray emission at E > 20 GeV, and thus particle acceleration, from GW sources. CTA will not be greatly limited by the precision of GW localization as it will be be capable of rapidly covering the GW error region with sufficient sensitivity. We examine the current status of GW searches and their follow-up effort, as well as the status of CTA, in order to identify some of the general strategies that will enhance CTA's contribution to multimessenger discoveries.
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subjects Error detection
Gamma rays
Gravitation
Gravitational waves
Particle acceleration
Physics - High Energy Astrophysical Phenomena
Telescopes
title Strategies for the Follow-up of Gravitational Wave Transients with the Cherenkov Telescope Array
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