The IceCube Collaboration -- Contributions to the 38th International Cosmic Ray Conference (ICRC2023)
The IceCube Observatory at the South Pole has been operating in its full configuration since May 2011 with a duty cycle of about 99%. Its main component consists of a cubic-kilometer array of optical sensors deployed deep in the Glacial ice designed for the detection of high-energy astrophysical neu...
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| creator | Abbasi, R Ashida, Y Axani, S. N Baricevic, M Bernardini, E Blot, S Bontempo, F Meneguolo, C. Boscolo Böser, S Böttcher, J Braun, J Brinson, B Butterfield, D Campana, M. A Chattopadhyay, S Chau, N Collin, G. H Coppin, P Desai, A Díaz-Vélez, J. C Domi, A Dujmovic, H Elsässer, D Evenson, P. A Farrag, K Fedynitch, A Finley, C Franckowiak, A Fürst, P Ganster, E Glüsenkamp, T Gray, S. J Gries, O Groth, K. M Günther, C Haack, C Halve, L Hanson, K Henningsen, F Heuermann, L Hidvegi, A Japaridze, G. S Kang, D Kang, W Kang, X Karl, M Zathul, A. Khatee Kontrimas, T Kopper, C Kovacevich, M Kowalski, M Kozynets, T Krishnamoorthi, J Kumar, A Lee, J. W Liubarska, M Lohfink, E Love, C Makino, Y Martinez-Soler, I Micallef, J Morii, Y Nagai, R Nakos, M Necker, J Negi, A Neumann, M Noell, A O'Dell, V Osborn, J Parker, G. K Rawlins, K Reichherzer, P Rhode, W Rodan, S Saffer, J Savelberg, J Savina, P Schneider, J Sharma, A Smithers, B Spiczak, G. M Spiering, C Taboada, I Ter-Antonyan, S Thompson, W. G Tilav, S Tosi, D Tung, C. F Upshaw, K van Santen, J Vara, J Veitch-Michaelis, J Weaver, C Weldert, J Witthaus, L Yildizci, E Young, R Yu, S Zhelnin, P |
| description | The IceCube Observatory at the South Pole has been operating in its full
configuration since May 2011 with a duty cycle of about 99%. Its main component
consists of a cubic-kilometer array of optical sensors deployed deep in the
Glacial ice designed for the detection of high-energy astrophysical neutrinos.
A surface array for cosmic ray air shower detection, IceTop, and a denser inner
subdetector, DeepCore, significantly enhance the capabilities of the
observatory, making it a multipurpose facility. This list of contributions to
the 38th International Cosmic Ray Conference in Nagoya, Japan (July 26 - August
3, 2023) summarizes the latest results from IceCube covering a broad set of key
questions in physics and astrophysics. The papers in this index are grouped
topically to highlight IceCube contributions related to high-energy neutrino
and multi-messenger astrophysics, cosmic-ray physics, low-energy neutrino
transients such as Galactic supernovae, fundamental physics, detector
calibration and event reconstruction, education and public outreach, and
research and development for the IceCube Upgrade, a scheduled dense sensor
infill complemented by calibration devices. Contributions related to
IceCube-Gen2, the future extension of IceCube, are available in a separate
collection. |
| doi_str_mv | 10.48550/arxiv.2307.13047 |
| format | Article |
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configuration since May 2011 with a duty cycle of about 99%. Its main component
consists of a cubic-kilometer array of optical sensors deployed deep in the
Glacial ice designed for the detection of high-energy astrophysical neutrinos.
A surface array for cosmic ray air shower detection, IceTop, and a denser inner
subdetector, DeepCore, significantly enhance the capabilities of the
observatory, making it a multipurpose facility. This list of contributions to
the 38th International Cosmic Ray Conference in Nagoya, Japan (July 26 - August
3, 2023) summarizes the latest results from IceCube covering a broad set of key
questions in physics and astrophysics. The papers in this index are grouped
topically to highlight IceCube contributions related to high-energy neutrino
and multi-messenger astrophysics, cosmic-ray physics, low-energy neutrino
transients such as Galactic supernovae, fundamental physics, detector
calibration and event reconstruction, education and public outreach, and
research and development for the IceCube Upgrade, a scheduled dense sensor
infill complemented by calibration devices. Contributions related to
IceCube-Gen2, the future extension of IceCube, are available in a separate
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configuration since May 2011 with a duty cycle of about 99%. Its main component
consists of a cubic-kilometer array of optical sensors deployed deep in the
Glacial ice designed for the detection of high-energy astrophysical neutrinos.
A surface array for cosmic ray air shower detection, IceTop, and a denser inner
subdetector, DeepCore, significantly enhance the capabilities of the
observatory, making it a multipurpose facility. This list of contributions to
the 38th International Cosmic Ray Conference in Nagoya, Japan (July 26 - August
3, 2023) summarizes the latest results from IceCube covering a broad set of key
questions in physics and astrophysics. The papers in this index are grouped
topically to highlight IceCube contributions related to high-energy neutrino
and multi-messenger astrophysics, cosmic-ray physics, low-energy neutrino
transients such as Galactic supernovae, fundamental physics, detector
calibration and event reconstruction, education and public outreach, and
research and development for the IceCube Upgrade, a scheduled dense sensor
infill complemented by calibration devices. Contributions related to
IceCube-Gen2, the future extension of IceCube, are available in a separate
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F ; Upshaw, K ; van Santen, J ; Vara, J ; Veitch-Michaelis, J ; Weaver, C ; Weldert, J ; Witthaus, L ; Yildizci, E ; Young, R ; Yu, S ; Zhelnin, P</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a677-6187a86345daaa642d48f2f67e1f76c96a30e395ab2c76310c7080b67168b0a13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Physics - High Energy Astrophysical Phenomena</topic><topic>Physics - Instrumentation and Methods for Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Abbasi, R</creatorcontrib><creatorcontrib>Ashida, Y</creatorcontrib><creatorcontrib>Axani, S. N</creatorcontrib><creatorcontrib>Baricevic, M</creatorcontrib><creatorcontrib>Bernardini, E</creatorcontrib><creatorcontrib>Blot, S</creatorcontrib><creatorcontrib>Bontempo, F</creatorcontrib><creatorcontrib>Meneguolo, C. 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A</creatorcontrib><creatorcontrib>Farrag, K</creatorcontrib><creatorcontrib>Fedynitch, A</creatorcontrib><creatorcontrib>Finley, C</creatorcontrib><creatorcontrib>Franckowiak, A</creatorcontrib><creatorcontrib>Fürst, P</creatorcontrib><creatorcontrib>Ganster, E</creatorcontrib><creatorcontrib>Glüsenkamp, T</creatorcontrib><creatorcontrib>Gray, S. J</creatorcontrib><creatorcontrib>Gries, O</creatorcontrib><creatorcontrib>Groth, K. M</creatorcontrib><creatorcontrib>Günther, C</creatorcontrib><creatorcontrib>Haack, C</creatorcontrib><creatorcontrib>Halve, L</creatorcontrib><creatorcontrib>Hanson, K</creatorcontrib><creatorcontrib>Henningsen, F</creatorcontrib><creatorcontrib>Heuermann, L</creatorcontrib><creatorcontrib>Hidvegi, A</creatorcontrib><creatorcontrib>Japaridze, G. S</creatorcontrib><creatorcontrib>Kang, D</creatorcontrib><creatorcontrib>Kang, W</creatorcontrib><creatorcontrib>Kang, X</creatorcontrib><creatorcontrib>Karl, M</creatorcontrib><creatorcontrib>Zathul, A. Khatee</creatorcontrib><creatorcontrib>Kontrimas, T</creatorcontrib><creatorcontrib>Kopper, C</creatorcontrib><creatorcontrib>Kovacevich, M</creatorcontrib><creatorcontrib>Kowalski, M</creatorcontrib><creatorcontrib>Kozynets, T</creatorcontrib><creatorcontrib>Krishnamoorthi, J</creatorcontrib><creatorcontrib>Kumar, A</creatorcontrib><creatorcontrib>Lee, J. W</creatorcontrib><creatorcontrib>Liubarska, M</creatorcontrib><creatorcontrib>Lohfink, E</creatorcontrib><creatorcontrib>Love, C</creatorcontrib><creatorcontrib>Makino, Y</creatorcontrib><creatorcontrib>Martinez-Soler, I</creatorcontrib><creatorcontrib>Micallef, J</creatorcontrib><creatorcontrib>Morii, Y</creatorcontrib><creatorcontrib>Nagai, R</creatorcontrib><creatorcontrib>Nakos, M</creatorcontrib><creatorcontrib>Necker, J</creatorcontrib><creatorcontrib>Negi, A</creatorcontrib><creatorcontrib>Neumann, M</creatorcontrib><creatorcontrib>Noell, A</creatorcontrib><creatorcontrib>O'Dell, V</creatorcontrib><creatorcontrib>Osborn, J</creatorcontrib><creatorcontrib>Parker, G. K</creatorcontrib><creatorcontrib>Rawlins, K</creatorcontrib><creatorcontrib>Reichherzer, P</creatorcontrib><creatorcontrib>Rhode, W</creatorcontrib><creatorcontrib>Rodan, S</creatorcontrib><creatorcontrib>Saffer, J</creatorcontrib><creatorcontrib>Savelberg, J</creatorcontrib><creatorcontrib>Savina, P</creatorcontrib><creatorcontrib>Schneider, J</creatorcontrib><creatorcontrib>Sharma, A</creatorcontrib><creatorcontrib>Smithers, B</creatorcontrib><creatorcontrib>Spiczak, G. M</creatorcontrib><creatorcontrib>Spiering, C</creatorcontrib><creatorcontrib>Taboada, I</creatorcontrib><creatorcontrib>Ter-Antonyan, S</creatorcontrib><creatorcontrib>Thompson, W. G</creatorcontrib><creatorcontrib>Tilav, S</creatorcontrib><creatorcontrib>Tosi, D</creatorcontrib><creatorcontrib>Tung, C. F</creatorcontrib><creatorcontrib>Upshaw, K</creatorcontrib><creatorcontrib>van Santen, J</creatorcontrib><creatorcontrib>Vara, J</creatorcontrib><creatorcontrib>Veitch-Michaelis, J</creatorcontrib><creatorcontrib>Weaver, C</creatorcontrib><creatorcontrib>Weldert, J</creatorcontrib><creatorcontrib>Witthaus, L</creatorcontrib><creatorcontrib>Yildizci, E</creatorcontrib><creatorcontrib>Young, R</creatorcontrib><creatorcontrib>Yu, S</creatorcontrib><creatorcontrib>Zhelnin, P</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Abbasi, R</au><au>Ashida, Y</au><au>Axani, S. N</au><au>Baricevic, M</au><au>Bernardini, E</au><au>Blot, S</au><au>Bontempo, F</au><au>Meneguolo, C. Boscolo</au><au>Böser, S</au><au>Böttcher, J</au><au>Braun, J</au><au>Brinson, B</au><au>Butterfield, D</au><au>Campana, M. A</au><au>Chattopadhyay, S</au><au>Chau, N</au><au>Collin, G. H</au><au>Coppin, P</au><au>Desai, A</au><au>Díaz-Vélez, J. C</au><au>Domi, A</au><au>Dujmovic, H</au><au>Elsässer, D</au><au>Evenson, P. A</au><au>Farrag, K</au><au>Fedynitch, A</au><au>Finley, C</au><au>Franckowiak, A</au><au>Fürst, P</au><au>Ganster, E</au><au>Glüsenkamp, T</au><au>Gray, S. J</au><au>Gries, O</au><au>Groth, K. M</au><au>Günther, C</au><au>Haack, C</au><au>Halve, L</au><au>Hanson, K</au><au>Henningsen, F</au><au>Heuermann, L</au><au>Hidvegi, A</au><au>Japaridze, G. S</au><au>Kang, D</au><au>Kang, W</au><au>Kang, X</au><au>Karl, M</au><au>Zathul, A. Khatee</au><au>Kontrimas, T</au><au>Kopper, C</au><au>Kovacevich, M</au><au>Kowalski, M</au><au>Kozynets, T</au><au>Krishnamoorthi, J</au><au>Kumar, A</au><au>Lee, J. W</au><au>Liubarska, M</au><au>Lohfink, E</au><au>Love, C</au><au>Makino, Y</au><au>Martinez-Soler, I</au><au>Micallef, J</au><au>Morii, Y</au><au>Nagai, R</au><au>Nakos, M</au><au>Necker, J</au><au>Negi, A</au><au>Neumann, M</au><au>Noell, A</au><au>O'Dell, V</au><au>Osborn, J</au><au>Parker, G. K</au><au>Rawlins, K</au><au>Reichherzer, P</au><au>Rhode, W</au><au>Rodan, S</au><au>Saffer, J</au><au>Savelberg, J</au><au>Savina, P</au><au>Schneider, J</au><au>Sharma, A</au><au>Smithers, B</au><au>Spiczak, G. M</au><au>Spiering, C</au><au>Taboada, I</au><au>Ter-Antonyan, S</au><au>Thompson, W. G</au><au>Tilav, S</au><au>Tosi, D</au><au>Tung, C. F</au><au>Upshaw, K</au><au>van Santen, J</au><au>Vara, J</au><au>Veitch-Michaelis, J</au><au>Weaver, C</au><au>Weldert, J</au><au>Witthaus, L</au><au>Yildizci, E</au><au>Young, R</au><au>Yu, S</au><au>Zhelnin, P</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The IceCube Collaboration -- Contributions to the 38th International Cosmic Ray Conference (ICRC2023)</atitle><date>2023-07-24</date><risdate>2023</risdate><abstract>The IceCube Observatory at the South Pole has been operating in its full
configuration since May 2011 with a duty cycle of about 99%. Its main component
consists of a cubic-kilometer array of optical sensors deployed deep in the
Glacial ice designed for the detection of high-energy astrophysical neutrinos.
A surface array for cosmic ray air shower detection, IceTop, and a denser inner
subdetector, DeepCore, significantly enhance the capabilities of the
observatory, making it a multipurpose facility. This list of contributions to
the 38th International Cosmic Ray Conference in Nagoya, Japan (July 26 - August
3, 2023) summarizes the latest results from IceCube covering a broad set of key
questions in physics and astrophysics. The papers in this index are grouped
topically to highlight IceCube contributions related to high-energy neutrino
and multi-messenger astrophysics, cosmic-ray physics, low-energy neutrino
transients such as Galactic supernovae, fundamental physics, detector
calibration and event reconstruction, education and public outreach, and
research and development for the IceCube Upgrade, a scheduled dense sensor
infill complemented by calibration devices. Contributions related to
IceCube-Gen2, the future extension of IceCube, are available in a separate
collection.</abstract><doi>10.48550/arxiv.2307.13047</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | DOI: 10.48550/arxiv.2307.13047 |
| ispartof | |
| issn | |
| language | eng |
| recordid | cdi_arxiv_primary_2307_13047 |
| source | arXiv.org |
| subjects | Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics |
| title | The IceCube Collaboration -- Contributions to the 38th International Cosmic Ray Conference (ICRC2023) |
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