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IceTop: The surface component of IceCube

Abstract:

IceTop, the surface component of the IceCube Neutrino Observatory at the South Pole, is an air shower array with an area of 1 km2. The detector allows a detailed exploration of the mass composition of primary cosmic rays in the energy range from about 100 TeV to 1 EeV by exploiting the correlation between the shower energy measured in IceTop and the energy deposited by muons in the deep ice. In this paper we report on the technical design, construction and installation, the trigger and data acquisition systems as well as the software framework for calibration, reconstruction and simulation. Finally the first experience from commissioning and operating the detector and the performance as an air shower detector will be discussed.

Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1016/j.nima.2012.10.067

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Publisher:
Elsevier
Journal:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment More from this journal
Volume:
700
Pages:
188-220
Publication date:
2012-10-27
Acceptance date:
2012-10-17
DOI:
EISSN:
1872-9576
ISSN:
0168-9002


Keywords:
Pubs id:
pubs:350363
UUID:
uuid:6ee27cbc-a15f-467d-898f-47fa4285316e
Local pid:
pubs:350363
Source identifiers:
350363
Deposit date:
2017-08-16
ARK identifier:

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