MEASUREMENT OF THE ANISOTROPY OF COSMIC-RAY ARRIVAL DIRECTIONS WITH ICECUBE
We report the first observation of an anisotropy in the arrival direction of cosmic rays with energies in the multi-TeV region in theSouthern sky using data from the IceCube detector. Between 2007 June and 2008 March, the partially deployed IceCube detector was operated in a configuration with 1320...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , |
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Format: | Journal article |
Language: | English |
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2010
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author | Abbasi, R Abdou, Y Abu-Zayyad, T Adams, J Aguilar, J Ahlers, M Andeen, K Auffenberg, J Bai, X Baker, M Barwick, S Bay, R Alba, J Beattie, K Beatty, J Bechet, S Becker, J Becker, K Benabderrahmane, M BenZvi, S Berdermann, J Berghaus, P Berley, D Bernardini, E Bertrand, D |
author_facet | Abbasi, R Abdou, Y Abu-Zayyad, T Adams, J Aguilar, J Ahlers, M Andeen, K Auffenberg, J Bai, X Baker, M Barwick, S Bay, R Alba, J Beattie, K Beatty, J Bechet, S Becker, J Becker, K Benabderrahmane, M BenZvi, S Berdermann, J Berghaus, P Berley, D Bernardini, E Bertrand, D |
author_sort | Abbasi, R |
collection | OXFORD |
description | We report the first observation of an anisotropy in the arrival direction of cosmic rays with energies in the multi-TeV region in theSouthern sky using data from the IceCube detector. Between 2007 June and 2008 March, the partially deployed IceCube detector was operated in a configuration with 1320 digital optical sensors distributed over22 strings at depths between 1450 and 2450 m inside the Antarctic ice. IceCube is a neutrino detector, but the data are dominated by a large background of cosmic-ray muons. Therefore, the background data aresuitable for high-statistics studies of cosmic rays in the southern sky. The data include 4.3 billion muons produced by downward-going cosmic-ray interactions in the atmosphere; these events were reconstructed with a median angular resolution of 3° and a median energy of ∼20 TeV. Their arrival direction distribution exhibits an anisotropy in right ascension with a first-harmonic amplitude of (6.4±0.2 stat.±0.8 syst.) × 10-4. © 2010 The American Astronomical Society. |
first_indexed | 2024-03-07T03:03:55Z |
format | Journal article |
id | oxford-uuid:b1e02fc0-ef4a-4c72-a811-1eeabb09732f |
institution | University of Oxford |
language | English |
last_indexed | 2024-03-07T03:03:55Z |
publishDate | 2010 |
record_format | dspace |
spelling | oxford-uuid:b1e02fc0-ef4a-4c72-a811-1eeabb09732f2022-03-27T04:07:24ZMEASUREMENT OF THE ANISOTROPY OF COSMIC-RAY ARRIVAL DIRECTIONS WITH ICECUBEJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:b1e02fc0-ef4a-4c72-a811-1eeabb09732fEnglishSymplectic Elements at Oxford2010Abbasi, RAbdou, YAbu-Zayyad, TAdams, JAguilar, JAhlers, MAndeen, KAuffenberg, JBai, XBaker, MBarwick, SBay, RAlba, JBeattie, KBeatty, JBechet, SBecker, JBecker, KBenabderrahmane, MBenZvi, SBerdermann, JBerghaus, PBerley, DBernardini, EBertrand, DWe report the first observation of an anisotropy in the arrival direction of cosmic rays with energies in the multi-TeV region in theSouthern sky using data from the IceCube detector. Between 2007 June and 2008 March, the partially deployed IceCube detector was operated in a configuration with 1320 digital optical sensors distributed over22 strings at depths between 1450 and 2450 m inside the Antarctic ice. IceCube is a neutrino detector, but the data are dominated by a large background of cosmic-ray muons. Therefore, the background data aresuitable for high-statistics studies of cosmic rays in the southern sky. The data include 4.3 billion muons produced by downward-going cosmic-ray interactions in the atmosphere; these events were reconstructed with a median angular resolution of 3° and a median energy of ∼20 TeV. Their arrival direction distribution exhibits an anisotropy in right ascension with a first-harmonic amplitude of (6.4±0.2 stat.±0.8 syst.) × 10-4. © 2010 The American Astronomical Society. |
spellingShingle | Abbasi, R Abdou, Y Abu-Zayyad, T Adams, J Aguilar, J Ahlers, M Andeen, K Auffenberg, J Bai, X Baker, M Barwick, S Bay, R Alba, J Beattie, K Beatty, J Bechet, S Becker, J Becker, K Benabderrahmane, M BenZvi, S Berdermann, J Berghaus, P Berley, D Bernardini, E Bertrand, D MEASUREMENT OF THE ANISOTROPY OF COSMIC-RAY ARRIVAL DIRECTIONS WITH ICECUBE |
title | MEASUREMENT OF THE ANISOTROPY OF COSMIC-RAY ARRIVAL DIRECTIONS WITH ICECUBE |
title_full | MEASUREMENT OF THE ANISOTROPY OF COSMIC-RAY ARRIVAL DIRECTIONS WITH ICECUBE |
title_fullStr | MEASUREMENT OF THE ANISOTROPY OF COSMIC-RAY ARRIVAL DIRECTIONS WITH ICECUBE |
title_full_unstemmed | MEASUREMENT OF THE ANISOTROPY OF COSMIC-RAY ARRIVAL DIRECTIONS WITH ICECUBE |
title_short | MEASUREMENT OF THE ANISOTROPY OF COSMIC-RAY ARRIVAL DIRECTIONS WITH ICECUBE |
title_sort | measurement of the anisotropy of cosmic ray arrival directions with icecube |
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