Follow-up of IceCube alerts with KM3NeT ARCA and ORCA
In this contribution, we present the follow-up of several recent IceCube real-time alerts of potential astrophysical neutrinos, using the complementarity of KM3NeT-ORCA and KM3NeT-ARCA data. Due to their geometry, these detectors cover a broad neutrino energy range, from few GeV to tens of PeV. At t...
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ftzenodo:oai:zenodo.org:6805372 2023-05-15T17:53:26+02:00 Follow-up of IceCube alerts with KM3NeT ARCA and ORCA Juan Palacios González 2022-07-07 https://zenodo.org/record/6805372 https://doi.org/10.5281/zenodo.6805372 unknown doi:10.5281/zenodo.6805371 https://zenodo.org/communities/neutrino2022-posters https://zenodo.org/record/6805372 https://doi.org/10.5281/zenodo.6805372 oai:zenodo.org:6805372 info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by/4.0/legalcode info:eu-repo/semantics/conferencePoster poster 2022 ftzenodo https://doi.org/10.5281/zenodo.680537210.5281/zenodo.6805371 2023-03-11T01:40:13Z In this contribution, we present the follow-up of several recent IceCube real-time alerts of potential astrophysical neutrinos, using the complementarity of KM3NeT-ORCA and KM3NeT-ARCA data. Due to their geometry, these detectors cover a broad neutrino energy range, from few GeV to tens of PeV. At the time of each alert, both detectors were in operation with partial configurations. Each follow-up has been performed by looking for a signal excess around the best Active Galactic Nuclei (AGN) counterpart position. A standard time window of ±1 day around the IceCube alerts, as well as an extended search time window of 1 month, have been tested. The analyses and their results, including statistical significance, are reported here. Conference Object Orca Zenodo |
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In this contribution, we present the follow-up of several recent IceCube real-time alerts of potential astrophysical neutrinos, using the complementarity of KM3NeT-ORCA and KM3NeT-ARCA data. Due to their geometry, these detectors cover a broad neutrino energy range, from few GeV to tens of PeV. At the time of each alert, both detectors were in operation with partial configurations. Each follow-up has been performed by looking for a signal excess around the best Active Galactic Nuclei (AGN) counterpart position. A standard time window of ±1 day around the IceCube alerts, as well as an extended search time window of 1 month, have been tested. The analyses and their results, including statistical significance, are reported here. |
format |
Conference Object |
author |
Juan Palacios González |
spellingShingle |
Juan Palacios González Follow-up of IceCube alerts with KM3NeT ARCA and ORCA |
author_facet |
Juan Palacios González |
author_sort |
Juan Palacios González |
title |
Follow-up of IceCube alerts with KM3NeT ARCA and ORCA |
title_short |
Follow-up of IceCube alerts with KM3NeT ARCA and ORCA |
title_full |
Follow-up of IceCube alerts with KM3NeT ARCA and ORCA |
title_fullStr |
Follow-up of IceCube alerts with KM3NeT ARCA and ORCA |
title_full_unstemmed |
Follow-up of IceCube alerts with KM3NeT ARCA and ORCA |
title_sort |
follow-up of icecube alerts with km3net arca and orca |
publishDate |
2022 |
url |
https://zenodo.org/record/6805372 https://doi.org/10.5281/zenodo.6805372 |
genre |
Orca |
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Orca |
op_relation |
doi:10.5281/zenodo.6805371 https://zenodo.org/communities/neutrino2022-posters https://zenodo.org/record/6805372 https://doi.org/10.5281/zenodo.6805372 oai:zenodo.org:6805372 |
op_rights |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by/4.0/legalcode |
op_doi |
https://doi.org/10.5281/zenodo.680537210.5281/zenodo.6805371 |
_version_ |
1766161138766053376 |