$F_{\gamma }$: a new observable for photon-hadron discrimination in hybrid air shower events

Abstract

To search for ultra-high-energy photons in primary cosmic rays, air shower observables are needed that allow a good separation between primary photons and primary hadrons. We present a new observable, $F_{\gamma }$, which can be extracted from ground-array data in hybrid events, where simultaneous measurements of the longitudinal and the lateral shower profile are performed. The observable is based on a template fit to the lateral distribution measured by the ground array with the template taking into account the complementary information from the measurement of the longitudinal profile, i.e. the primary energy and the geometry of the shower. $F_{\gamma }$ shows a very good photon-hadron separation, which is even superior to the separation given by the well-known $X_{\text{max}}$ observable (the atmospheric depth of the shower maximum). At energies around $1\text{EeV}$ ($10\text{EeV}$), $F_{\gamma }$ provides a background rejection better than $97.8\%$ ($99.9\%$) at a signal efficiency of $50\%$. Advantages of the observable $F_{\gamma }$ are its technical stability with respect to irregularities in the ground array (i.e. missing or temporarily non-operating stations) and that it can be applied over the full energy range accessible to the air shower detector, down to its threshold energy. Furthermore, $F_{\gamma }$ complements nicely to $X_{\text{max}}$ such that both observables can well be combined to achieve an even better discrimination power, exploiting the rich information available in hybrid events.

10 pages, 6 figures; v2: added journal reference

References in corpus (11)

• Depth of Maximum of Air-Shower Profiles at the Pierre Auger Observatory: Measurements at Energies above 10^17.8 eV
• One-dimensional Hybrid Approach to Extensive Air Shower Simulation
• The Offline Software Framework of the Pierre Auger Observatory
• Radio detection of Cosmic-Ray Air Showers and High-Energy Neutrinos
• Search for ultra-high energy photons using air showers
• The Optimum Distance at which to Determine the Size of a Giant Air Shower
• A search for point sources of EeV photons
• A targeted search for point sources of EeV photons with the Pierre Auger Observatory
• The Pierre Auger Observatory III: Other Astrophysical Observations
• Changes in extensive air showers from isotropic Lorentz violation in the photon sector
• Potential sensitivities to Lorentz violation from nonbirefringent modified Maxwell theory of Auger, HESS, and CTA

Cited by in corpus (1)

• EmCa -- Electromagnetic-Cascades Simulation Package