Capabilities of IceCube's gamma-ray, optical and X-ray follow-up programs

The IceCube neutrino observatory is a 1 km3 detector for Cherenkov light in the ice at the South Pole. Although the presence of a diffuse astrophysical neutrino flux has been confirmed, its origin has yet to be resolved. Given the current constraints on continuous point source searches, transient an...

Full description

Bibliographic Details
Published in:EPJ Web of Conferences
Main Author: Kintscher Thomas
Format: Article in Journal/Newspaper
Language:English
Published: EDP Sciences 2016
Subjects:
Online Access:https://doi.org/10.1051/epjconf/201611610002
https://doaj.org/article/36220f8050ea4461b5bbafb79160013b
id ftdoajarticles:oai:doaj.org/article:36220f8050ea4461b5bbafb79160013b
record_format openpolar
spelling ftdoajarticles:oai:doaj.org/article:36220f8050ea4461b5bbafb79160013b 2023-05-15T18:22:09+02:00 Capabilities of IceCube's gamma-ray, optical and X-ray follow-up programs Kintscher Thomas 2016-01-01T00:00:00Z https://doi.org/10.1051/epjconf/201611610002 https://doaj.org/article/36220f8050ea4461b5bbafb79160013b EN eng EDP Sciences http://dx.doi.org/10.1051/epjconf/201611610002 https://doaj.org/toc/2100-014X 2100-014X doi:10.1051/epjconf/201611610002 https://doaj.org/article/36220f8050ea4461b5bbafb79160013b EPJ Web of Conferences, Vol 116, p 10002 (2016) Physics QC1-999 article 2016 ftdoajarticles https://doi.org/10.1051/epjconf/201611610002 2022-12-31T15:28:57Z The IceCube neutrino observatory is a 1 km3 detector for Cherenkov light in the ice at the South Pole. Although the presence of a diffuse astrophysical neutrino flux has been confirmed, its origin has yet to be resolved. Given the current constraints on continuous point source searches, transient and variable objects emerge as promising, detectable source candidates. IceCube boosts the sensitivity to these types of sources by alerting third-party observatories of neutrino events clustered in direction and time. This paper will showcase several neutrino-triggered multi-messenger programs in IceCube along with their results and prospects. Article in Journal/Newspaper South pole Directory of Open Access Journals: DOAJ Articles South Pole EPJ Web of Conferences 116 10002
institution Open Polar
collection Directory of Open Access Journals: DOAJ Articles
op_collection_id ftdoajarticles
language English
topic Physics
QC1-999
spellingShingle Physics
QC1-999
Kintscher Thomas
Capabilities of IceCube's gamma-ray, optical and X-ray follow-up programs
topic_facet Physics
QC1-999
description The IceCube neutrino observatory is a 1 km3 detector for Cherenkov light in the ice at the South Pole. Although the presence of a diffuse astrophysical neutrino flux has been confirmed, its origin has yet to be resolved. Given the current constraints on continuous point source searches, transient and variable objects emerge as promising, detectable source candidates. IceCube boosts the sensitivity to these types of sources by alerting third-party observatories of neutrino events clustered in direction and time. This paper will showcase several neutrino-triggered multi-messenger programs in IceCube along with their results and prospects.
format Article in Journal/Newspaper
author Kintscher Thomas
author_facet Kintscher Thomas
author_sort Kintscher Thomas
title Capabilities of IceCube's gamma-ray, optical and X-ray follow-up programs
title_short Capabilities of IceCube's gamma-ray, optical and X-ray follow-up programs
title_full Capabilities of IceCube's gamma-ray, optical and X-ray follow-up programs
title_fullStr Capabilities of IceCube's gamma-ray, optical and X-ray follow-up programs
title_full_unstemmed Capabilities of IceCube's gamma-ray, optical and X-ray follow-up programs
title_sort capabilities of icecube's gamma-ray, optical and x-ray follow-up programs
publisher EDP Sciences
publishDate 2016
url https://doi.org/10.1051/epjconf/201611610002
https://doaj.org/article/36220f8050ea4461b5bbafb79160013b
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_source EPJ Web of Conferences, Vol 116, p 10002 (2016)
op_relation http://dx.doi.org/10.1051/epjconf/201611610002
https://doaj.org/toc/2100-014X
2100-014X
doi:10.1051/epjconf/201611610002
https://doaj.org/article/36220f8050ea4461b5bbafb79160013b
op_doi https://doi.org/10.1051/epjconf/201611610002
container_title EPJ Web of Conferences
container_volume 116
container_start_page 10002
_version_ 1766201507674324992