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  • A Search for Photons with E...
    Almela, A.; Anastasi, G. A.; Anchordoqui, L.; Aramo, C.; Arnone, E.; Balaceanu, A.; Biteau, J.; Bleve, C.; Blümer, J.; Boncioli, D.; Arbeletche, L. Bonneau; Borodai, N.; Brack, J.; Orchera, P. G. Brichetto; Büsken, M.; Canfora, F.; Catalani, F.; Colalillo, R.; Condorelli, A.; Dasso, S.; Dawson, B. R.; de Jong, S. J.; de Souza, V.; dos Anjos, R. C.; Etchegoyen, A.; Falcke, H.; Farmer, J.; Fujii, T.; Galelli, C.; Giammarchi, M.; Glombitza, J.; Gollan, F.; Gorgi, A.; Guarino, F.; Guido, E.; Harvey, V. M.; Heck, D.; Janecek, P.; Jurysek, J.; Kampert, K. H.; Keilhauer, B.; Khakurdikar, A.; Kleifges, M.; Presti, D. Lo; López, R.; Lundquist, J. P.; Mandat, D.; Manning, B. C.; Manshanden, J.; Marafico, S.; Mariazzi, A. G.; Martinelli, S.; Mollerach, S.; Müller, A. L.; Mulrey, K.; Nasr-Esfahani, A.; Nellen, L.; Nitz, D.; Nosek, D.; Nožka, L.; Papenbreer, P.; Pech, M.; Peña-Rodriguez, J.; Perrone, L.; Petrucci, C.; Pimenta, M.; Pirronello, V.; Pothast, M.; Prouza, M.; Puyleart, A.; Querchfeld, S.; Rojo, J. Rodriguez; Rovero, A. C.; Salamida, F.; Salazar, H.; Gomez, J. D. Sanabria; Sánchez, F.; Sarazin, F.; Scherini, V.; Scholten, O.; Schulte, J.; Shellard, R. C.; Sima, O.; Smau, R.; Soriano, J. F.; Squartini, R.; Stasielak, J.; Suomijärvi, T.; Timmermans, C.; Torrès, Z.; Unger, M.; Vaclavek, L.; Vacula, M.; Vásquez-Ramírez, A.; Quispe, I. D. Vergara; Vink, J.; Wahlberg, H.; Yushkov, A.; Zavrtanik, M.; Zehrer, L.

    The Astrophysical journal, 07/2022, Letnik: 933, Številka: 2
    Journal Article

    Abstract Ultra-high-energy photons with energies exceeding 10 17 eV offer a wealth of connections to different aspects of cosmic-ray astrophysics as well as to gamma-ray and neutrino astronomy. The recent observations of photons with energies in the 10 15 eV range further motivate searches for even higher-energy photons. In this paper, we present a search for photons with energies exceeding 2 × 10 17 eV using about 5.5 yr of hybrid data from the low-energy extensions of the Pierre Auger Observatory. The upper limits on the integral photon flux derived here are the most stringent ones to date in the energy region between 10 17 and 10 18 eV.