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Title:A search for ultra-high-energy photons at the Pierre Auger Observatory exploiting air-shower universality
Authors:ID Savina, P. (Author)
ID Filipčič, Andrej (Author)
ID Lundquist, Jon Paul (Author)
ID Stanič, Samo (Author)
ID Vorobiov, Serguei (Author)
ID Zavrtanik, Danilo (Author)
ID Zavrtanik, Marko (Author)
ID Zehrer, Lukas (Author), et al.
Files:.pdf ICRC2021_373.pdf (1,12 MB)
MD5: 684CBF853C105593CDB53D791E99CC69
 
URL https://pos.sissa.it/395/373/
 
URL https://pos.sissa.it/395/373/pdf
 
Language:English
Work type:Not categorized
Typology:1.08 - Published Scientific Conference Contribution
Organization:UNG - University of Nova Gorica
Abstract:The Pierre Auger Observatory is the most sensitive detector to primary photons with energies above ∼ 0.2 EeV. It measures extensive air showers using a hybrid technique that combines a fluorescence detector (FD) with a ground array of particle detectors (SD). The signatures of a photon-induced air shower are a larger atmospheric depth at the shower maximum (Xmax) and a steeper lateral distribution function, along with a lower number of muons with respect to the bulk of hadron-induced background. Using observables measured by the FD and SD, three photon searches in different energy bands are performed. In particular, between threshold energies of 1–10 EeV, a new analysis technique has been developed by combining the FD-based measurement of Xmax with the SD signal through a parameter related to its muon content, derived from the universality of the air showers. This technique has led to a better photon/hadron separation and, consequently, to a higher search sensitivity, resulting in a tighter upper limit than before. The outcome of this new analysis is presented here, along with previous results in the energy ranges below 1 EeV and above 10 EeV. From the data collected by the Pierre Auger Observatory in about 15 years of operation, the most stringent constraints on the fraction of photons in the cosmic flux are set over almost three decades in energy.
Keywords:Pierre Auger Observatory, indirect detection, fluorescence detection, surface array, hybrid detection, ultra-high energy, cosmic rays, photons
Publication status:Published
Year of publishing:2022
PID:20.500.12556/RUNG-8481 New window
COBISS.SI-ID:166312963 New window
DOI:https://doi.org/10.22323/1.395.0373 New window
NUK URN:URN:SI:UNG:REP:1CT3KJOY
Publication date in RUNG:29.09.2023
Views:731
Downloads:5
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Record is a part of a monograph

Title:37th International Cosmic Ray Conference : ICRC2023
Place of publishing:Trieste, Italy
Publisher:Proceedings of Science
Year of publishing:2022

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