Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-02-21
Phys.Rev.Lett. 95 (2005) 171102
Astronomy and Astrophysics
Astrophysics
4 pages, 3 figures. Analysis extended to account for primary energy resolution; conclusions unchanged. Accepted by Phys. Rev.
Scientific paper
10.1103/PhysRevLett.95.171102
A new method to derive an upper limit on photon primaries from small data sets of air showers is developed which accounts for shower properties varying with the primary energy and arrival direction. Applying this method to the highest-energy showers recorded by the AGASA experiment, an upper limit on the photon fraction of 51% (67%) at a confidence level of 90% (95%) for primary energies above 1.25 * 10^20 eV is set. This new limit on the photon fraction above the GZK cutoff energy constrains the Z-burst model of the origin of highest-energy cosmic rays.
Engel R. R.
Góra Dariusz
Heck Dieter
Homola Piotr
Pȩkala Jan
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