The IceCube realtime alert system
© 2017 Elsevier B.V. Although high-energy astrophysical neutrinos were discovered in 2013, their origin is still unknown. Aiming for the identification of an electromagnetic counterpart of a rapidly fading source, we have implemented a realtime analysis framework for the IceCube neutrino observatory...
Published in: | Astroparticle Physics |
---|---|
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format: | Article in Journal/Newspaper |
Language: | English |
Published: |
eScholarship, University of California
2017
|
Subjects: | |
Online Access: | http://www.escholarship.org/uc/item/5kt749cn |
id |
ftcdlib:qt5kt749cn |
---|---|
record_format |
openpolar |
spelling |
ftcdlib:qt5kt749cn 2023-05-15T13:43:56+02:00 The IceCube realtime alert system Aartsen, MG Ackermann, M Adams, J Aguilar, JA Ahlers, M Ahrens, M Altmann, D Andeen, K Anderson, T Ansseau, I Anton, G Archinger, M Argüelles, C Auffenberg, J Axani, S Bai, X Barwick, SW Baum, V Bay, R Beatty, JJ Becker Tjus, J Becker, KH BenZvi, S Berley, D Bernardini, E Bernhard, A Besson, DZ Binder, G Bindig, D Bissok, M Blaufuss, E Blot, S Bohm, C Börner, M Bos, F Bose, D Böser, S Botner, O Braun, J Brayeur, L Bretz, HP Bron, S Burgman, A Carver, T Casier, M Cheung, E Chirkin, D Christov, A Clark, K Classen, L Coenders, S Collin, GH Conrad, JM Cowen, DF Cross, R Day, M de André, JPAM De Clercq, C del Pino Rosendo, E Dembinski, H De Ridder, S Desiati, P de Vries, KD de Wasseige, G de With, M DeYoung, T Díaz-Vélez, JC di Lorenzo, V Dujmovic, H Dumm, JP Dunkman, M Eberhardt, B Ehrhardt, T Eichmann, B Eller, P Euler, S Evenson, PA Fahey, S Fazely, AR Feintzeig, J Felde, J Filimonov, K Finley, C Flis, S Fösig, CC Franckowiak, A Friedman, E Fuchs, T Gaisser, TK Gallagher, J Gerhardt, L Ghorbani, K Giang, W Gladstone, L Glauch, T Glüsenkamp, T 30 - 41 2017-06-01 application/pdf http://www.escholarship.org/uc/item/5kt749cn english eng eScholarship, University of California qt5kt749cn http://www.escholarship.org/uc/item/5kt749cn public Aartsen, MG; Ackermann, M; Adams, J; Aguilar, JA; Ahlers, M; Ahrens, M; et al.(2017). The IceCube realtime alert system. Astroparticle Physics, 92, 30 - 41. doi:10.1016/j.astropartphys.2017.05.002. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/5kt749cn article 2017 ftcdlib https://doi.org/10.1016/j.astropartphys.2017.05.002 2018-07-13T22:57:50Z © 2017 Elsevier B.V. Although high-energy astrophysical neutrinos were discovered in 2013, their origin is still unknown. Aiming for the identification of an electromagnetic counterpart of a rapidly fading source, we have implemented a realtime analysis framework for the IceCube neutrino observatory. Several analyses selecting neutrinos of astrophysical origin are now operating in realtime at the detector site in Antarctica and are producing alerts for the community to enable rapid follow-up observations. The goal of these observations is to locate the astrophysical objects responsible for these neutrino signals. This paper highlights the infrastructure in place both at the South Pole site and at IceCube facilities in the north that have enabled this fast follow-up program to be implemented. Additionally, this paper presents the first realtime analyses to be activated within this framework, highlights their sensitivities to astrophysical neutrinos and background event rates, and presents an outlook for future discoveries. Article in Journal/Newspaper Antarc* Antarctica South pole South pole University of California: eScholarship South Pole Astroparticle Physics 92 30 41 |
institution |
Open Polar |
collection |
University of California: eScholarship |
op_collection_id |
ftcdlib |
language |
English |
description |
© 2017 Elsevier B.V. Although high-energy astrophysical neutrinos were discovered in 2013, their origin is still unknown. Aiming for the identification of an electromagnetic counterpart of a rapidly fading source, we have implemented a realtime analysis framework for the IceCube neutrino observatory. Several analyses selecting neutrinos of astrophysical origin are now operating in realtime at the detector site in Antarctica and are producing alerts for the community to enable rapid follow-up observations. The goal of these observations is to locate the astrophysical objects responsible for these neutrino signals. This paper highlights the infrastructure in place both at the South Pole site and at IceCube facilities in the north that have enabled this fast follow-up program to be implemented. Additionally, this paper presents the first realtime analyses to be activated within this framework, highlights their sensitivities to astrophysical neutrinos and background event rates, and presents an outlook for future discoveries. |
format |
Article in Journal/Newspaper |
author |
Aartsen, MG Ackermann, M Adams, J Aguilar, JA Ahlers, M Ahrens, M Altmann, D Andeen, K Anderson, T Ansseau, I Anton, G Archinger, M Argüelles, C Auffenberg, J Axani, S Bai, X Barwick, SW Baum, V Bay, R Beatty, JJ Becker Tjus, J Becker, KH BenZvi, S Berley, D Bernardini, E Bernhard, A Besson, DZ Binder, G Bindig, D Bissok, M Blaufuss, E Blot, S Bohm, C Börner, M Bos, F Bose, D Böser, S Botner, O Braun, J Brayeur, L Bretz, HP Bron, S Burgman, A Carver, T Casier, M Cheung, E Chirkin, D Christov, A Clark, K Classen, L Coenders, S Collin, GH Conrad, JM Cowen, DF Cross, R Day, M de André, JPAM De Clercq, C del Pino Rosendo, E Dembinski, H De Ridder, S Desiati, P de Vries, KD de Wasseige, G de With, M DeYoung, T Díaz-Vélez, JC di Lorenzo, V Dujmovic, H Dumm, JP Dunkman, M Eberhardt, B Ehrhardt, T Eichmann, B Eller, P Euler, S Evenson, PA Fahey, S Fazely, AR Feintzeig, J Felde, J Filimonov, K Finley, C Flis, S Fösig, CC Franckowiak, A Friedman, E Fuchs, T Gaisser, TK Gallagher, J Gerhardt, L Ghorbani, K Giang, W Gladstone, L Glauch, T Glüsenkamp, T |
spellingShingle |
Aartsen, MG Ackermann, M Adams, J Aguilar, JA Ahlers, M Ahrens, M Altmann, D Andeen, K Anderson, T Ansseau, I Anton, G Archinger, M Argüelles, C Auffenberg, J Axani, S Bai, X Barwick, SW Baum, V Bay, R Beatty, JJ Becker Tjus, J Becker, KH BenZvi, S Berley, D Bernardini, E Bernhard, A Besson, DZ Binder, G Bindig, D Bissok, M Blaufuss, E Blot, S Bohm, C Börner, M Bos, F Bose, D Böser, S Botner, O Braun, J Brayeur, L Bretz, HP Bron, S Burgman, A Carver, T Casier, M Cheung, E Chirkin, D Christov, A Clark, K Classen, L Coenders, S Collin, GH Conrad, JM Cowen, DF Cross, R Day, M de André, JPAM De Clercq, C del Pino Rosendo, E Dembinski, H De Ridder, S Desiati, P de Vries, KD de Wasseige, G de With, M DeYoung, T Díaz-Vélez, JC di Lorenzo, V Dujmovic, H Dumm, JP Dunkman, M Eberhardt, B Ehrhardt, T Eichmann, B Eller, P Euler, S Evenson, PA Fahey, S Fazely, AR Feintzeig, J Felde, J Filimonov, K Finley, C Flis, S Fösig, CC Franckowiak, A Friedman, E Fuchs, T Gaisser, TK Gallagher, J Gerhardt, L Ghorbani, K Giang, W Gladstone, L Glauch, T Glüsenkamp, T The IceCube realtime alert system |
author_facet |
Aartsen, MG Ackermann, M Adams, J Aguilar, JA Ahlers, M Ahrens, M Altmann, D Andeen, K Anderson, T Ansseau, I Anton, G Archinger, M Argüelles, C Auffenberg, J Axani, S Bai, X Barwick, SW Baum, V Bay, R Beatty, JJ Becker Tjus, J Becker, KH BenZvi, S Berley, D Bernardini, E Bernhard, A Besson, DZ Binder, G Bindig, D Bissok, M Blaufuss, E Blot, S Bohm, C Börner, M Bos, F Bose, D Böser, S Botner, O Braun, J Brayeur, L Bretz, HP Bron, S Burgman, A Carver, T Casier, M Cheung, E Chirkin, D Christov, A Clark, K Classen, L Coenders, S Collin, GH Conrad, JM Cowen, DF Cross, R Day, M de André, JPAM De Clercq, C del Pino Rosendo, E Dembinski, H De Ridder, S Desiati, P de Vries, KD de Wasseige, G de With, M DeYoung, T Díaz-Vélez, JC di Lorenzo, V Dujmovic, H Dumm, JP Dunkman, M Eberhardt, B Ehrhardt, T Eichmann, B Eller, P Euler, S Evenson, PA Fahey, S Fazely, AR Feintzeig, J Felde, J Filimonov, K Finley, C Flis, S Fösig, CC Franckowiak, A Friedman, E Fuchs, T Gaisser, TK Gallagher, J Gerhardt, L Ghorbani, K Giang, W Gladstone, L Glauch, T Glüsenkamp, T |
author_sort |
Aartsen, MG |
title |
The IceCube realtime alert system |
title_short |
The IceCube realtime alert system |
title_full |
The IceCube realtime alert system |
title_fullStr |
The IceCube realtime alert system |
title_full_unstemmed |
The IceCube realtime alert system |
title_sort |
icecube realtime alert system |
publisher |
eScholarship, University of California |
publishDate |
2017 |
url |
http://www.escholarship.org/uc/item/5kt749cn |
op_coverage |
30 - 41 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
Antarc* Antarctica South pole South pole |
genre_facet |
Antarc* Antarctica South pole South pole |
op_source |
Aartsen, MG; Ackermann, M; Adams, J; Aguilar, JA; Ahlers, M; Ahrens, M; et al.(2017). The IceCube realtime alert system. Astroparticle Physics, 92, 30 - 41. doi:10.1016/j.astropartphys.2017.05.002. Lawrence Berkeley National Laboratory: Retrieved from: http://www.escholarship.org/uc/item/5kt749cn |
op_relation |
qt5kt749cn http://www.escholarship.org/uc/item/5kt749cn |
op_rights |
public |
op_doi |
https://doi.org/10.1016/j.astropartphys.2017.05.002 |
container_title |
Astroparticle Physics |
container_volume |
92 |
container_start_page |
30 |
op_container_end_page |
41 |
_version_ |
1766195191854661632 |