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    The design and performance of IceCube DeepCore

    Access Status
    Fulltext not available
    Authors
    Abbasi, R.
    Abdou, Y.
    Abu-Zayyad, T.
    Ackermann, M.
    Adams, J.
    Aguilar, J.
    Ahlers, M.
    Allen, M.
    Altmann, D.
    Andeen, K.
    Auffenberg, J.
    Bai, X.
    Baker, M.
    Barwick, S.
    Bay, R.
    Bazo 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.
    Besson, D.
    Bindig, D.
    Bissok, M.
    Blaufuss, E.
    Blumenthal, J.
    Boersma, D.
    Bohm, C.
    Bose, D.
    Böser, S.
    Botner, O.
    Brown, A.
    Buitink, S.
    Caballero-Mora, K.
    Carson, Michael
    Chirkin, D.
    Christy, B.
    Clevermann, F.
    Cohen, S.
    Colnard, C.
    Cowen, D.
    Cruz Silva, A.
    D'Agostino, M.
    Danninger, M.
    Daughhetee, J.
    Davis, J.
    De Clercq, C.
    Degner, T.
    Demirörs, L.
    Descamps, F.
    Desiati, P.
    De Vries-Uiterweerd, G.
    Deyoung, T.
    Díaz-Vélez, J.
    Dierckxsens, M.
    Dreyer, J.
    Dumm, J.
    Dunkman, M.
    Eisch, J.
    Ellsworth, R.
    Engdegrd, O.
    Euler, S.
    Evenson, P.
    Fadiran, O.
    Fazely, A.
    Fedynitch, A.
    Feintzeig, J.
    Feusels, T.
    Filimonov, K.
    Finley, C.
    Fischer-Wasels, T.
    Fox, B.
    Franckowiak, A.
    Franke, R.
    Gaisser, T.
    Gallagher, J.
    Gerhardt, L.
    Gladstone, L.
    Glüsenkamp, T.
    Goldschmidt, A.
    Goodman, J.
    Góra, D.
    Grant, D.
    Griesel, T.
    Groß, A.
    Grullon, S.
    Gurtner, M.
    Date
    2012
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Abbasi, R. and Abdou, Y. and Abu-Zayyad, T. and Ackermann, M. and Adams, J. and Aguilar, J. and Ahlers, M. et al. 2012. The design and performance of IceCube DeepCore. Astroparticle Physics. 35 (10): pp. 615-624.
    Source Title
    Astroparticle Physics
    DOI
    10.1016/j.astropartphys.2012.01.004
    ISSN
    0927-6505
    School
    Department of Exploration Geophysics
    URI
    http://hdl.handle.net/20.500.11937/6493
    Collection
    • Curtin Research Publications
    Abstract

    The IceCube neutrino observatory in operation at the South Pole, Antarctica, comprises three distinct components: a large buried array for ultrahigh energy neutrino detection, a surface air shower array, and a new buried component called DeepCore. DeepCore was designed to lower the IceCube neutrino energy threshold by over an order of magnitude, to energies as low as about 10 GeV. DeepCore is situated primarily 2100 m below the surface of the icecap at the South Pole, at the bottom center of the existing IceCube array, and began taking physics data in May 2010. Its location takes advantage of the exceptionally clear ice at those depths and allows it to use the surrounding IceCube detector as a highly efficient active veto against the principal background of downward-going muons produced in cosmic-ray air showers. DeepCore has a module density roughly five times higher than that of the standard IceCube array, and uses photomultiplier tubes with a new photocathode featuring a quantum efficiency about 35% higher than standard IceCube PMTs. Taken together, these features of DeepCore will increase IceCube’s sensitivity to neutrinos from WIMP dark matter annihilations, atmospheric neutrino oscillations, galactic supernova neutrinos, and point sources of neutrinos in the northern and southern skies. In this paper we describe the design and initial performance of DeepCore.

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