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The SNEWS 2.0 Alert Software for the Coincident Detection of Neutrinos from Core-Collapse Supernovae

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arxiv 2406.17743 v2 pith:4T4L535L submitted 2024-06-25 astro-ph.IM astro-ph.HE

classification astro-ph.IMastro-ph.HE
keywords snewsalertdetectorsnetworkneutrinosystemcoincidentcombined
verification ladder T0 review T1 audit T2 compute T3 formal

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The neutrino signal from the next galactic core-collapse supernova will provide an invaluable early warning of the explosion. By combining the burst trigger from several neutrino detectors, the location of the explosion can be triangulated minutes to hours before the optical emission becomes visible, while also reducing the rate of false-positive triggers. To enable multi-messenger follow-up of nearby supernovae, the SuperNova Early Warning System 2.0 (SNEWS 2.0) will produce a combined alert using a global network of neutrino detectors. This paper describes the trigger publishing and alert formation framework of the SNEWS 2.0 network. The framework is built on the HOPSKOTCH publish-subscribe system to easily incorporate new detectors into the network, and it implements a coincidence system to form alerts and estimate a false-positive rate for the combined triggers. The paper outlines the structure of the SNEWS 2.0 software and the initial testing of coincident signals.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope

    astro-ph.IM 2026-07 accept novelty 6.0 of 10

    Degrading the Einstein Telescope's sensitivity in specific frequency bands hurts different science goals in predictable ways, but the mission remains scientifically strong even in the worst modelled cases.

  2. Enhanced antineutrino emission from $\beta$ decay in core-collapse supernovae with self-consistent weak decay rates

    astro-ph.HE 2025-11 conditional novelty 6.0 of 10

    Adding microscopic beta-decay rates to supernova simulations makes the pre-bounce antineutrino signal orders of magnitude brighter than positron-capture-only models.

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