Astrophysics Motivation behind the Pierre Auger Southern Observatory Enhancements

Abstract

The Pierre Auger Collaboration intends to extend the energy range of its southern observatory in Argentina for high quality data from 0.1 to 3 EeV. The extensions, described in accompanying papers, include three additional fluorescence telescopes with a more elevated field of view (HEAT) and a nested surface array with 750 and 433 m spacing respectively and additional muon detection capabilities (AMIGA). The enhancement of the detector will allow measurement of cosmic rays, using the same techniques, from below the second knee up to the highest energies observed. The evolution of the spectrum through the second knee and ankle, and corresponding predicted changes in composition, are crucial to the understanding of the end of Galactic confinement and the effects of propagation on the lower energy portion of the extragalactic flux. The latter is strongly related to the cosmological distribution of sources and to the composition of the injected spectrum. We discuss the science motivation behind these enhancements as well as the impact of combined HEAT and AMIGA information on the assessment of shower simulations and reconstruction techniques.

Proc. of the 30th Int. Cosmic Ray Conference, Merida, Mexico, July 2007

Cited by in corpus (6)

• Cherenkov Flashes and Fluorescence Flares on Telescopes: New lights on UHECR Spectroscopy while unveiling Neutrinos Astronomy
• Reconstruction of air shower muon densities using segmented counters with time resolution
• Estimation of the number of muons with muon counters
• The Pierre Auger Observatory - a new stage in the study of the ultra-high energy cosmic rays
• Energy determination of cosmic ray showers in surface arrays using signal inference at a single distance from the core
• A method to reconstruct the muon lateral distribution with an array of segmented counters with time resolution