English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Plus monthly

Global: Zendy Tools annual

Global: Zendy Tools monthly

Global: Zendy Free Plan

The IceCube Neutrino Observatory, which instruments 1$\,$km$^3$ of clear iceat the geographic South Pole, was mainly designed to detect particles withenergies in the multi-GeV to PeV range. Due to ice temperatures between$-20^\circ$C to $-43^\circ$C and the low radioactivity of the ice, the darknoise rates of the 5160 photomultiplier tubes forming the IceCube lattice areof order 500 Hz, which is particularly low for 10 inch photomultipliers.Therefore, IceCube can extend its searches to bursts of$\mathcal{O}$(10$\,$MeV) neutrinos lasting several seconds, which are expectedto be produced by Galactic core collapse supernovae. By observing a uniformrise in all photomultiplier rates, IceCube can provide a particularly highstatistical precision for the neutrino rate from supernovae in the inner partof our Galaxy ($<$ 20 kpc). In this paper, the tools and the method to studypotential obscured or failed core collapse supernovae in our Galaxy arepresented. The analysis will be based on 3911 days of IceCube data takenbetween April 17, 2008 and December 31, 2018.

Eleven Year Search for Supernovae with the IceCube Neutrino Observatory