Capabilities of IceCube’s Gamma-Ray, Optical and X-Ray Follow-Up Programs
The IceCube neutrino observatory is a 1 km$^3$ 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...
| Published in: | EPJ Web of Conferences |
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| Main Author: | |
| Format: | Conference Object |
| Language: | English |
| Published: |
EDP Sciences
2015
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| Subjects: | |
| Online Access: | https://bib-pubdb1.desy.de/record/293511 https://bib-pubdb1.desy.de/search?p=id:%22PUBDB-2016-00593%22 |
| _version_ | 1821714872488951808 |
|---|---|
| author | Kintscher, Thomas |
| author_facet | Kintscher, Thomas |
| author_sort | Kintscher, Thomas |
| collection | DESY Publication Database (PUBDB) |
| container_start_page | 10002 |
| container_title | EPJ Web of Conferences |
| container_volume | 116 |
| description | The IceCube neutrino observatory is a 1 km$^3$ 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 | Conference Object |
| genre | South pole |
| genre_facet | South pole |
| geographic | South Pole |
| geographic_facet | South Pole |
| id | ftdesyvdb:oai:bib-pubdb1.desy.de:293511 |
| institution | Open Polar |
| language | English |
| op_collection_id | ftdesyvdb |
| op_coverage | DE |
| op_doi | https://doi.org/10.1051/epjconf/201611610002 |
| op_relation | info:eu-repo/semantics/altIdentifier/wos/WOS:000386965400063 info:eu-repo/semantics/altIdentifier/doi/10.1051/epjconf/201611610002 info:eu-repo/semantics/altIdentifier/issn/2100-014X https://bib-pubdb1.desy.de/record/293511 https://bib-pubdb1.desy.de/search?p=id:%22PUBDB-2016-00593%22 |
| op_rights | info:eu-repo/semantics/closedAccess |
| op_source | The European physical journal / Web of Conferences 116, 10002 (2015). doi:10.1051/epjconf/201611610002 Very Large Volume Neutrino Telescope Workshop, VLVnT-2015, La Sapienza, Italy, 2015-09-14 - 2015-09-16 |
| publishDate | 2015 |
| publisher | EDP Sciences |
| record_format | openpolar |
| spelling | ftdesyvdb:oai:bib-pubdb1.desy.de:293511 2025-01-17T00:51:33+00:00 Capabilities of IceCube’s Gamma-Ray, Optical and X-Ray Follow-Up Programs Kintscher, Thomas DE 2015 https://bib-pubdb1.desy.de/record/293511 https://bib-pubdb1.desy.de/search?p=id:%22PUBDB-2016-00593%22 eng eng EDP Sciences info:eu-repo/semantics/altIdentifier/wos/WOS:000386965400063 info:eu-repo/semantics/altIdentifier/doi/10.1051/epjconf/201611610002 info:eu-repo/semantics/altIdentifier/issn/2100-014X https://bib-pubdb1.desy.de/record/293511 https://bib-pubdb1.desy.de/search?p=id:%22PUBDB-2016-00593%22 info:eu-repo/semantics/closedAccess The European physical journal / Web of Conferences 116, 10002 (2015). doi:10.1051/epjconf/201611610002 Very Large Volume Neutrino Telescope Workshop, VLVnT-2015, La Sapienza, Italy, 2015-09-14 - 2015-09-16 info:eu-repo/classification/ddc/530 info:eu-repo/semantics/conferenceObject info:eu-repo/semantics/publishedVersion 2015 ftdesyvdb https://doi.org/10.1051/epjconf/201611610002 2022-06-30T20:13:30Z The IceCube neutrino observatory is a 1 km$^3$ 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. Conference Object South pole DESY Publication Database (PUBDB) South Pole EPJ Web of Conferences 116 10002 |
| spellingShingle | info:eu-repo/classification/ddc/530 Kintscher, Thomas Capabilities of IceCube’s Gamma-Ray, Optical and X-Ray Follow-Up Programs |
| title | 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_short | 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 |
| topic | info:eu-repo/classification/ddc/530 |
| topic_facet | info:eu-repo/classification/ddc/530 |
| url | https://bib-pubdb1.desy.de/record/293511 https://bib-pubdb1.desy.de/search?p=id:%22PUBDB-2016-00593%22 |