The HiRes prototype detector with 14 mirrors has been operational for more than two years. Some air showers are observed in coincidence with other detectors (CASA, MIA, FE2, HiRes2). However, here we examine the larger data set which includes showers observed by the HiRes prototype alone. We describe the analysis techniques of shower reconstruction for the monocular data. Preliminary distributions are reported. We have also done a pilot study search for point sources. 1. Geometrical reconstruction The shower track and the detector determine a plane called the "tra kd tector plane. " The technique for finding that plane is described by Bird et al.[1]. The track within the plane has to be determined by the phototube firing times in ...
The CLUE experiment studies primary cosmic rays (E > 2 TeV) by detecting UV (190-230 nm) Cherenkov l...
The High Altitude Water Cherenkov (HAWC) gamma-ray observatory is a ground-based air shower array de...
The surface detector array of the Pierre Auger Observatory consists of 1600 water-Cherenkov detector...
The HiRes prototype detector is now observing extensive air showers above 50 PeV in coincidence with...
International audienceWe have studied several sources of systematic uncertainty in calculating the a...
Abstract: A method to calculate the Average Longitudinal Shower profile has been applied to the High...
At ground level, surface detector arrays sample the secondary particles from extensive air showers i...
Ground-based gamma-ray astronomy aims at reconstructing the energy and direction of gamma rays from ...
Located in the western desert of the state of Utah, the Telescope Array (TA) experiment measures the...
The CLUE UV C~erenkov telescope array has started to take data with 8 telescopes in January 1998. Th...
International audienceThe High Energy Stereoscopic System (H.E.S.S.) is an array of five Imaging Atm...
Copyright © 2004 Elsevier B.V. All rights reserved.In the past few years, small scale anisotropy has...
The CLUE experiment studies primary cosmic rays (E > 2 TeV) by detecting UV (190-230 nm) Cherenkov l...
The High Altitude Water Cherenkov (HAWC) gamma-ray observatory is a ground-based air shower array de...
The surface detector array of the Pierre Auger Observatory consists of 1600 water-Cherenkov detector...
The HiRes prototype detector is now observing extensive air showers above 50 PeV in coincidence with...
International audienceWe have studied several sources of systematic uncertainty in calculating the a...
Abstract: A method to calculate the Average Longitudinal Shower profile has been applied to the High...
At ground level, surface detector arrays sample the secondary particles from extensive air showers i...
Ground-based gamma-ray astronomy aims at reconstructing the energy and direction of gamma rays from ...
Located in the western desert of the state of Utah, the Telescope Array (TA) experiment measures the...
The CLUE UV C~erenkov telescope array has started to take data with 8 telescopes in January 1998. Th...
International audienceThe High Energy Stereoscopic System (H.E.S.S.) is an array of five Imaging Atm...
Copyright © 2004 Elsevier B.V. All rights reserved.In the past few years, small scale anisotropy has...
The CLUE experiment studies primary cosmic rays (E > 2 TeV) by detecting UV (190-230 nm) Cherenkov l...
The High Altitude Water Cherenkov (HAWC) gamma-ray observatory is a ground-based air shower array de...
The surface detector array of the Pierre Auger Observatory consists of 1600 water-Cherenkov detector...