P. Allison, J. Bellido, X. Bertou, C. E. Covault, B. E. Fick, H. Gemmeke, ...
of the Pierre Auger Observatory requires accurate timing (25 nanoseconds or better) between measurements at individual detectors and instrument triggers. Timing systems for both SD and FD are based...
The Auger Fluorescence Detector Prototype Telescope (2007)
H. Bluemer, V. Bocci, J. Castro E, R. Cester, A. Cordero, P. Facal, ...
The Pierre Auger Cosmic Ray Observatory will study cosmic rays above 10 EeV using both atmospheric fluorescence measurements and ground level particle detectors. A demonstration hybrid observatory...
Allison, P., Bellido, J., Bertou, X., Fick, B.E., Gemmeke, H., Kleifges, M., ...
29th Internat.Cosmic Ray Conf., Poona, IND, August 3-10, 2005
Abu-Zayyad, T., Belov, K., Cao, Z., Chen, G.F., Dai, H.Y., Elbert, J.W., ...
The average extensive air shower longitudinal development profile is measured. Events between 10 17 and 10 18 eV recorded by the HiRes/MIA hybrid experiment are used for the average profile. Several...
Abu-Zayyad, T., Belov, K., Bird, D. J., Boyer, J., Cao, Z., Catanese, M., ...
Copyright © 2001 Elsevier Science B.V. All rights reserved.
Abu-Zayyad, T., Belov, K., Bird, D. J., Boyer, J., Cao, Z., Catanese, M., ...
© 2001. The American Astronomical Society
Abu-Zayyad, T., Belov, K., Bird, D. J., Boyer, J., Cao, Z., Catanese, M., ...
Copyright © 2001 Elsevier Science B.V. All rights reserved.
Abu-Zayyad, T., Belov, K., Bird, D. J., Boyer, J., Cao, Z., Catanese, M., ...
© 2001. The American Astronomical Society
Abu-Zayyad, T., Belov, K., Cao, Z., Chen, G.F., Dai, H.Y., Elbert, J.W., ...
The average extensive air shower longitudinal development profile is measured. Events between 10 17 and 10 18 eV recorded by the HiRes/MIA hybrid experiment are used for the average profile. Several...
Abu-Zayyad, T., Belov, K., Cao, Z., Chen, G.F., Dai, H.Y., Elbert, J.W., ...
The average extensive air shower longitudinal development profile is measured. Events between 10 17 and 10 18 eV recorded by the HiRes/MIA hybrid experiment are used for the average profile. Several...
Abu-Zayyad, T., Belov, K., Cao, Z., Chen, G.F., Dai, H.Y., Elbert, J.W., ...
The average extensive air shower longitudinal development profile is measured. Events between 10 17 and 10 18 eV recorded by the HiRes/MIA hybrid experiment are used for the average profile. Several...
Abu-Zayyad, T., Belov, K., Bird, D. J., Boyer, J., Cao, Z., Catanese, M., ...
We study the spectrum and average mass composition of cosmic rays with primary energies between 10^{17} eV and 10^{18} eV using a hybrid detector consisting of the High Resolution Fly's Eye (HiRes)...
Energy estimation of UHE cosmic rays using the atmospheric fluorescence technique (2000)
Song, C., Cao, Z., Dawson, Bruce Robert, Fick, B. E., Sokolsky, P., Zhang, X. Z.
Submitted to Cornell University’s online archive www.arxiv.org in 1999 by Chihwa Song
Abu-Zayyad, T., Belov, K., Bird, D. J., Boyer, J., Cao, Z., Catanese, M., ...
Copyright © 2000 The American Physical Society
Energy estimation of UHE cosmic rays using the atmospheric fluorescence technique (2000)
Song, C., Cao, Z., Dawson, Bruce Robert, Fick, B. E., Sokolsky, P., Zhang, X. Z.
Submitted to Cornell University’s online archive www.arxiv.org in 1999 by Chihwa Song
Abu-Zayyad, T., Belov, K., Bird, D. J., Boyer, J., Cao, Z., Catanese, M., ...
Copyright © 2000 The American Physical Society
A Multi-Component Measurement of the Cosmic Ray Composition Between 10^{17} eV and 10^{18} eV (1999)
Abu-Zayyad, T., Belov, K., Bird, D. J., Boyer, J., Cao, Z., Catanese, M., ...
The average mass composition of cosmic rays with primary energies between $10^{17}$eV and $10^{18}$eV has been studied using a hybrid detector consisting of the High Resolution Fly's Eye (HiRes)...
Energy Estimation of UHE Cosmic Rays using the Atmospheric Fluorescence Technique (1999)
Song, C., Cao, Z., Dawson, B. R., Fick, B. E., Sokolsky, P., Zhang, X.
We use the CORSIKA air shower simulation program to review the method for assigning energies to ultra-high energy (UHE) cosmic rays viewed with the air fluorescence technique. This technique uses the...
Constraints on Gamma-ray Emission from the Galactic Plane at 300 TeV (1997)
Borione, A., Catanese, M. A., Chantell, M. C., Covault, C. E., Cronin, J. W., Fick, B. E., ...
We describe a new search for diffuse ultrahigh energy gamma-ray emission associated with molecular clouds in the galactic disk. The Chicago Air Shower Array (CASA), operating in coincidence with the...
Borione, A., Covault, C. E., Cronin, J. W., Fick, B. E., Gibbs, K. G., Krimm, H. A., ...
We describe the technical details and the performance of a large array which detects both the electron and muon components in extensive air showers with energies >= 1014 eV. The array was designed...
The Cosmic Ray Energy Spectrum between 10^14 and 10^16 eV
M. A. Catanese, M.C. Chantell, C.E. Covault, J.W. Cronin, B. E. Fick, ...
The energy spectrum of cosmic rays with primary energies between 10 14 eV and 10 16 eV has been studied with the CASA-MIA air shower array. The measured differential energy spectrum is a power law...