Conference proceeding
Towards a cosmic ray composition measurement with the IceAct telescopes at the IceCube Neutrino Observatory
Pos : proceedings of science, v 444, 237
27 Sep 2024
Abstract
The IceCube Neutrino Observatory is equipped with the unique possibility to measure cosmic ray induced air showers simultaneously by their particle footprint on the surface with the IceTop detector and by the high-energy muonic shower component at a depth of more than 1.5 km. Since 2019 additionally, two Imaging Air Cherenkov Telescopes, called IceAct, measure the electromagnetic component of air showers in the atmosphere above the IceCube detector. This opens the possibility to measure air shower parameters in three independent detectors and allows to improve mass composition studies with the IceCube data. One IceAct camera consists of 61 SiPM pixels in a hexagonal grid. Each pixel has a field of view of 1.5 degree resulting in an approximately 12-degree field of view per camera. A single telescope tube has a diameter of 50 cm, is built robust enough to withstand the harsh Antarctic conditions, and is able to detect cosmic ray particles with energies above approximately 10 TeV. A Graph Neural Network (GNN) is trained to determine the air shower properties from IceAct data. The composition analysis is then performed using Random Forest Regression (RF). Since all three detectors have a different energy threshold, we train several RFs with different inputs, combining the different detectors and taking advantage of the lower energy threshold of the IceAct telescopes. This will result in composition measurements for different detector combinations and enables cross-checks of the results in overlapping energy bands. We present the method, parameters for data selection, and the status of this analysis.
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Details
- Title
- Towards a cosmic ray composition measurement with the IceAct telescopes at the IceCube Neutrino Observatory
- Creators
- Larissa Paul - South Dakota School of Mines and TechnologyR. Abbasi - Loyola University ChicagoM. Ackermann - Deutsches Elektronen-Synchrotron DESYJ. Adams - University of CanterburyS. K. Agarwalla - Institute of Physics, Bhubaneswar, IndiaJ. A. Aguilar - Université Libre de BruxellesM. Ahlers - University of CopenhagenJ. M. Alameddine - TU Dortmund UniversityN. M. Amin - University of DelawareK. Andeen - Marquette UniversityG. Anton - Friedrich-Alexander-Universität Erlangen-NürnbergC. Argüelles - Harvard UniversityY. Ashida - University of UtahS. Athanasiadou - Deutsches Elektronen-Synchrotron DESYS. N. Axani - University of DelawareX. Bai - South Dakota School of Mines and TechnologyA. V. Balagopal - University of Wisconsin–MadisonM. Baricevic - University of Wisconsin–MadisonS. W. Barwick - University of California, IrvineV. Basu - University of Wisconsin–MadisonR. Bay - University of California, BerkeleyJ. J. Beatty - The Ohio State UniversityJ. Becker Tjus - Chalmers University of TechnologyJ. Beise - Uppsala UniversityC. Bellenghi - Technical University of MunichC. Benning - RWTH Aachen UniversityS. BenZvi - University of RochesterD. Berley - University of Maryland, College ParkE. Bernardini - Dipartimento di Fisica e Astronomia Galileo Galilei, Università Degli Studi di Padova, Padova, ItalyD. Z. Besson - University of KansasE. Blaufuss - University of Maryland, College ParkS. Blot - Deutsches Elektronen-Synchrotron DESYF. Bontempo - Karlsruhe Institute of Technology, Institute for Astroparticle Physics, Karlsruhe, GermanyJ. Y. Book - Harvard UniversityC. Boscolo Meneguolo - Dipartimento di Fisica e Astronomia Galileo Galilei, Università Degli Studi di Padova, Padova, ItalyS. Böser - Institute of Physics, University of Mainz, Mainz, GermanyO. Botner - Uppsala UniversityJ. Böttcher - RWTH Aachen UniversityE. Bourbeau - University of CopenhagenJ. Braun - University of Wisconsin–MadisonT. Bretz - GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt, GermanyB. Brinson - Georgia Institute of TechnologyJ. Brostean-Kaiser - Deutsches Elektronen-Synchrotron DESYR. T. Burley - Department of Physics, University of Adelaide, Adelaide, AustraliaR. S. Busse - University of MünsterD. Butterfield - University of Wisconsin–MadisonM. A. Campana - Dept. of Physics, Drexel University, Philadelphia, PA, United StatesK. Carloni - Harvard UniversityE. G. Carnie-Bronca - The University of AdelaideS. Chattopadhyay - Institute of Physics, Bhubaneswar, IndiaN. Chau - Université Libre de BruxellesC. Chen - Georgia Institute of TechnologyZ. Chen - Stony Brook UniversityD. Chirkin - University of Wisconsin–MadisonS. Choi - Sungkyunkwan UniversityB. A. Clark - University of Maryland, College ParkL. Classen - University of MünsterA. Coleman - Uppsala UniversityG. H. Collin - Massachusetts Institute of TechnologyA. Connolly - The Ohio State UniversityJ. M. Conrad - Massachusetts Institute of TechnologyP. Coppin - Vrije Universiteit BrusselP. Correa - Vrije Universiteit BrusselD. F. Cowen - Pennsylvania State UniversityP. Dave - Georgia Institute of TechnologyC. De Clercq - Vrije Universiteit BrusselJ. J. DeLaunay - University of AlabamaD. Delgado - Harvard UniversityS. Deng - RWTH Aachen UniversityK. Deoskar - Stockholm UniversityA. Desai - University of Wisconsin–MadisonP. Desiati - University of Wisconsin–MadisonK. D. de Vries - Vrije Universiteit BrusselG. de Wasseige - UCLouvainT. DeYoung - Michigan State UniversityA. Diaz - Massachusetts Institute of TechnologyJ. C. Díaz-Vélez - University of Wisconsin–MadisonM. Dittmer - University of MünsterA. Domi - Friedrich-Alexander-Universität Erlangen-NürnbergH. Dujmovic - University of Wisconsin–MadisonM. A. DuVernois - University of Wisconsin–MadisonT. Ehrhardt - Institute of Physics, University of Mainz, Mainz, GermanyP. Eller - Technical University of MunichE. Ellinger - University of WuppertalS. El Mentawi - RWTH Aachen UniversityD. Elsässer - TU Dortmund UniversityR. Engel - Karlsruhe Institute of Technology, Institute of Experimental Particle Physics, Karlsruhe, GermanyH. Erpenbeck - University of Wisconsin–MadisonJ. Evans - University of Maryland, College ParkP. A. Evenson - University of DelawareK. L. Fan - University of Maryland, College ParkK. Fang - University of Wisconsin–MadisonK. Farrag - Chiba UniversityA. R. Fazely - Dept. of Physics, Southern University, Baton Rouge, LA, United StatesA. Fedynitch - Institute of Physics, Academia SinicaN. Feigl - Humboldt-Universität zu BerlinS. Fiedlschuster - Friedrich-Alexander-Universität Erlangen-NürnbergC. Finley - Stockholm UniversityL. Fischer - Deutsches Elektronen-Synchrotron DESYD. Fox - Pennsylvania State University
- Publication Details
- Pos : proceedings of science, v 444, 237
- Publisher
- Proceedings of Science
- Grant note
- Michigan State University (http://data.elsevier.com/vocabulary/SciValFunders/100007709) Helmholtz Association (http://data.elsevier.com/vocabulary/SciValFunders/501100009318) Fonds Wetenschappelijk Onderzoek (http://data.elsevier.com/vocabulary/SciValFunders/501100003130) Wisconsin Alumni Research Foundation (100001395) Marsden Fund (http://data.elsevier.com/vocabulary/SciValFunders/501100009193) Natural Sciences and Engineering Research Council of Canada (501100000038) University of Oxford (501100000769) Australian Research Council (http://data.elsevier.com/vocabulary/SciValFunders/501100000923) Bundesministerium für Bildung und Forschung (http://data.elsevier.com/vocabulary/SciValFunders/501100002347) U.S. National Science Foundation-Physics Division
- Resource Type
- Conference proceeding
- Language
- English
- Academic Unit
- Physics
- Scopus ID
- 2-s2.0-85212263269
- Other Identifier
- 991022202084704721