Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/82150
Type: Thesis
Title: Systematic and statistical uncertainties in cosmic ray arrival direction reconstruction.
Author: Wahrlich, Philip Shane
Issue Date: 2013
School/Discipline: School of Chemistry and Physics
Abstract: The Pierre Auger Observatory (PAO) was constructed to study the highest energy cosmic rays (UHECR). A hybrid of ground array and fluorescence detector, it is the largest ultra-high energy cosmic ray detector to date. As such, the PAO detects UHECR in unprecedented amounts, offering unique insights into the nature and origin of these most extraordinarily energetic particles in the universe. In this thesis we improve the accuracy of arrival direction uncertainty estimates for reconstructed events. We validate these improved uncertainty estimators through a number of statistical techniques, involving both recorded and simulated data. Furthermore, we identify and correct a number of systematic errors which arise in algorithmic corner cases. We propose novel techniques for measuring the time synchronisation of each detector in the using recorded air shower data. We use these techniques to measure the synchronisation of each detector across the PAO surface detector and fluorescence detector. Finally, we perform a cursory search for a point source of UHECR at the Galactic centre. A slight over-density of events is measured from the direction of the Galactic centre, however this over-density is not substantial enough to indicate a departure from isotropy.
Advisor: Dawson, Bruce Robert
Clay, Roger William
Dissertation Note: Thesis (Ph.D.)--University of Adelaide, School of Chemistry and Physics, 2013
Keywords: cosmic ray; UHECR; astrophysics; reconstruction
Provenance: Copyright material removed from digital thesis. See print copy in University of Adelaide Library for full text.
Appears in Collections:Research Theses

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