Follow-up of astrophysical transients in real time with the IceCube Neutrino Observatory

IceCube Collaboration, Pablo Correa Camiroaga, Catherine De Clercq, Krijn De Vries

Onderzoeksoutput: Articlepeer review

11 Citaten (Scopus)
84 Downloads (Pure)


In multi-messenger astronomy, rapid investigation of interesting transients is imperative. As an observatory with a 4$\pi$ steradian field of view and $\sim$99\% uptime, the IceCube Neutrino Observatory is a unique facility to follow up transients, and to provide valuable insight for other observatories and inform their observing decisions. Since 2016, IceCube has been using low-latency data to rapidly respond to interesting astrophysical events reported by the multi-messenger observational community. Here, we describe the pipeline used to perform these follow up analyses and provide a summary of the 58 analyses performed as of July 2020. We find no significant signal in the first 58 analyses performed. The pipeline has helped inform various electromagnetic observing strategies, and has constrained neutrino emission from potential hadronic cosmic accelerators.
Originele taal-2English
Aantal pagina's14
TijdschriftThe Astrophysical Journal
Nummer van het tijdschrift1
StatusPublished - 20 mrt 2021

Bibliografische nota

18 pages, 9 figures


Duik in de onderzoeksthema's van 'Follow-up of astrophysical transients in real time with the IceCube Neutrino Observatory'. Samen vormen ze een unieke vingerafdruk.

Citeer dit