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 x 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.

A Search for Photons with Energies Above 2 x 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory / Abreu, P; Aglietta, M; Albury, Jm; Allekotte, ; Cheminant, Ka; Almela, A; Alvarez-Muñiz, J; Batista, Ra; Yebra, Ja; Anastasi, Ga; Anchordoqui, L; Andrada, B; Andringa, S; Aramo, C; Ferreira, Pra; Arnone, E; Velázquez, Jca; Asorey, H; Assis, P; Avila, G; Avocone, E; Badescu, Am; Bakalova, A; Balaceanu, A; Barbato, F; Bellido, Ja; Berat, C; Bertaina, Me; Bhatta, G; Biermann, Pl; Binet, ; Bismark, K; Bister, T; Biteau, J; Blazek, J; Bleve, C; Blümer, J; Boncioli, D; Bonifazi, C; Arbeletche, Lb; Borodai, N; Botti, Am; Brack, J; Bretz, T; Orchera, Pgb; Briechle, Fl; Buchholz, P; Bueno, A; Buitink, S; Buscemi, M; Büsken, M; Caballero-Mora, Ks; Caccianiga, L; Canfora, F; Caracas, ; Caruso, R; Castellina, A; Catalani, F; Cataldi, G; Cazon, L; Cerda, M; Chinellato, Ja; Chudoba, J; Chytka, L; Clay, Rw; Cerutti, Acc; Colalillo, R; Coleman, A; Coluccia, Mr; Conceiçao, R; Condorelli, A; Consolati, G; Contreras, F; Convenga, F; Dos Santos, Dc; Covault, Ce; Dasso, S; Daumiller, K; Dawson, Br; Day, Ja; De Almeida, Rm; De Jesús, J; De Jong, Sj; Neto, Jrtd; De, Mitri; De Oliveira, J; Franco, Dd; De Palma, F; De, Souza; De Vito, E; Del Popolo, A; Del Río, M; Deligny, O; Deval, L; Di Matteo, A; Dobre, M; Dobrigkeit, C; Mendes, Lmd; Dos Anjos, Rc; Dova, Mt; Ebr, J; Engel, R; Epicoco, ; Erdmann, M; Escobar, Co; Etchegoyen, A; Falcke, H; Farmer, J; Farrar, G; Fauth, Ac; Fazzini, N; Feldbusch, F; Fenu, F; Fick, B; Figueira, Jm; Fitoussi, T; Fodran, T; Fujii, T; Fuster, A; Galea, C; Galelli, C; García, B; Vegas, Alg; Gemmeke, H; Gesualdi, F; Gherghel-Lascu, A; Ghia, Pl; Giaccari, U; Giammarchi, M; Glombitza, J; Gobbi, F; Gollan, F; Golup, G; Berisso, Mg; Vitale, Pfg; Gongora, Jp; González, Jm; González, N; Goos, ; Góra, D; Gorgi, A; Gottowik, M; Grubb, Td; Guarino, F; Guedes, Gp; Guido, E; Hahn, S; Hamal, P; Hampel, Mr; Hansen, P; Harari, D; Harvey, Vm; Haungs, A; Hebbeker, T; Heck, D; Hill, Gc; Hojvat, C; Hörandel, Jr; Horvath, P; Hrabovsky, M; Huege, T; Insolia, A; Isar, Pg; Janecek, P; Johnsen, Ja; Jurysek, J; Kääpä, A; Kampert, Kh; Keilhauer, B; Khakurdikar, A; Covilakam, Vvk; Klages, Ho; Kleifges, M; Kleinfeller, J; Knapp, F; Kunka, N; Lago, Bl; Langner, N; De Oliveira, Mal; Lenok, ; Letessier-Selvon, A; Lhenry-Yvon, ; Lo Presti, D; Lopes, L; López, R; Lu, L; Luce, Q; Lundquist, Jp; Payeras, Am; Mancarella, G; Mandat, D; Manning, Bc; Manshanden, J; Mantsch, P; Marafico, S; Mariani, Fm; Mariazzi, Ag; Marsella, G; Martello, D; Martinelli, S; Bravo, Om; Mastrodicasa, M; Mathes, Hj; Matthews, J; Matthiae, G; Mayotte, E; Mayotte, S; Mazur, Po; Medina-Tanco, G; Melo, D; Menshikov, A; Michal, S; Micheletti, M; Miramonti, L; Mollerach, S; Montanet, F; Morejon, L; Morello, C; Mostafá, M; Müller, Al; Muller, Ma; Mulrey, K; Mussa, R; Muzio, M; Namasaka, Wm; Nasr-Esfahani, A; Nellen, L; Nicora, G; Niculescu-Oglinzanu, M; Niechciol, M; Nitz, D; Norwood, ; Nosek, D; Novotny, ; Nozka, L; Nucita, A; Núñez, La; Oliveira, C; Palatka, M; Pallotta, J; Papenbreer, P; Parente, G; Parra, A; Pawlowsky, J; Pech, M; Pelayo, R; Peña-Rodriguez, J; Martins, Eep; Armand, Jp; Bertolli, Cp; Perrone, L; Petrera, S; Petrucci, C; Pierog, T; Pimenta, M; Pirronello, ; Platino, M; Pont, B; Pothast, M; Privitera, P; Prouza, M; Puyleart, A; Querchfeld, S; Rautenberg, J; Ravignani, D; Reininghaus, M; Ridky, J; Riehn, F; Risse, M; Rizi, ; De Carvalho, Wr; Rojo, Jr; Roncoroni, Mj; Rossoni, S; Roth, M; Roulet, E; Rovero, Ac; Ruehl, P; Saftoiu, A; Saharan, M; Salamida, F; Salazar, H; Salina, G; Gomez, Jds; Sánchez, F; Santos, Em; Santos, E; Sarazin, F; Sarmento, R; Sarmiento-Cano, C; Sato, R; Savina, P; Schäfer, Cm; Scherini, ; Schieler, H; Schimassek, M; Schimp, M; Schlüter, F; Schmidt, D; Scholten, O; Schoorlemmer, H; Schovánek, P; Schröder, Fg; Schulte, J; Schulz, T; Sciutto, Sj; Scornavacche, M; Segreto, A; Sehgal, S; Shellard, Rc; Sigl, G; Silli, G; Sima, O; Smau, R; Smída, R; Sommers, P; Soriano, Jf; Squartini, R; Stadelmaier, M; Stanca, D; Stasielak, J; Stassi, P; Streich, A; Suárez-Durán, M; Sudholz, T; Suomijärvi, T; Supanitsky, Ad; Szadkowski, Z; Tapia, A; Taricco, C; Timmermans, C; Tkachenko, O; Tobiska, P; Peixoto, Cjt; Tomé, B; Torrès, Z; Travaini, A; Travnicek, P; Trimarelli, C; Tueros, M; Ulrich, R; Unger, M; Vaclavek, L; Vacula, M; Galicia, Jfv; Valore, L; Varela, E; Vásquez-Ramírez, A; Ventura, C; Quispe, Idv; Verzi, V; Vicha, J; Vink, J; Vorobiov, S; Wahlberg, H; Watanabe, C; Watson, Aa; Weindl, A; Wiencke, L; Wittkowski, D; Wundheiler, B; Yushkov, A; Zapparrata, O; Zas, E; Zavrtanik, D; Zavrtanik, M; Zehrer, L. - In: THE ASTROPHYSICAL JOURNAL. - ISSN 0004-637X. - 933:2(2022). [10.3847/1538-4357/ac7393]

A Search for Photons with Energies Above 2 x 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory

Mastrodicasa, M;
2022

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 x 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.
2022
pierre auger observatory; photons; hybrid data
01 Pubblicazione su rivista::01a Articolo in rivista
A Search for Photons with Energies Above 2 x 1017 eV Using Hybrid Data from the Low-Energy Extensions of the Pierre Auger Observatory / Abreu, P; Aglietta, M; Albury, Jm; Allekotte, ; Cheminant, Ka; Almela, A; Alvarez-Muñiz, J; Batista, Ra; Yebra, Ja; Anastasi, Ga; Anchordoqui, L; Andrada, B; Andringa, S; Aramo, C; Ferreira, Pra; Arnone, E; Velázquez, Jca; Asorey, H; Assis, P; Avila, G; Avocone, E; Badescu, Am; Bakalova, A; Balaceanu, A; Barbato, F; Bellido, Ja; Berat, C; Bertaina, Me; Bhatta, G; Biermann, Pl; Binet, ; Bismark, K; Bister, T; Biteau, J; Blazek, J; Bleve, C; Blümer, J; Boncioli, D; Bonifazi, C; Arbeletche, Lb; Borodai, N; Botti, Am; Brack, J; Bretz, T; Orchera, Pgb; Briechle, Fl; Buchholz, P; Bueno, A; Buitink, S; Buscemi, M; Büsken, M; Caballero-Mora, Ks; Caccianiga, L; Canfora, F; Caracas, ; Caruso, R; Castellina, A; Catalani, F; Cataldi, G; Cazon, L; Cerda, M; Chinellato, Ja; Chudoba, J; Chytka, L; Clay, Rw; Cerutti, Acc; Colalillo, R; Coleman, A; Coluccia, Mr; Conceiçao, R; Condorelli, A; Consolati, G; Contreras, F; Convenga, F; Dos Santos, Dc; Covault, Ce; Dasso, S; Daumiller, K; Dawson, Br; Day, Ja; De Almeida, Rm; De Jesús, J; De Jong, Sj; Neto, Jrtd; De, Mitri; De Oliveira, J; Franco, Dd; De Palma, F; De, Souza; De Vito, E; Del Popolo, A; Del Río, M; Deligny, O; Deval, L; Di Matteo, A; Dobre, M; Dobrigkeit, C; Mendes, Lmd; Dos Anjos, Rc; Dova, Mt; Ebr, J; Engel, R; Epicoco, ; Erdmann, M; Escobar, Co; Etchegoyen, A; Falcke, H; Farmer, J; Farrar, G; Fauth, Ac; Fazzini, N; Feldbusch, F; Fenu, F; Fick, B; Figueira, Jm; Fitoussi, T; Fodran, T; Fujii, T; Fuster, A; Galea, C; Galelli, C; García, B; Vegas, Alg; Gemmeke, H; Gesualdi, F; Gherghel-Lascu, A; Ghia, Pl; Giaccari, U; Giammarchi, M; Glombitza, J; Gobbi, F; Gollan, F; Golup, G; Berisso, Mg; Vitale, Pfg; Gongora, Jp; González, Jm; González, N; Goos, ; Góra, D; Gorgi, A; Gottowik, M; Grubb, Td; Guarino, F; Guedes, Gp; Guido, E; Hahn, S; Hamal, P; Hampel, Mr; Hansen, P; Harari, D; Harvey, Vm; Haungs, A; Hebbeker, T; Heck, D; Hill, Gc; Hojvat, C; Hörandel, Jr; Horvath, P; Hrabovsky, M; Huege, T; Insolia, A; Isar, Pg; Janecek, P; Johnsen, Ja; Jurysek, J; Kääpä, A; Kampert, Kh; Keilhauer, B; Khakurdikar, A; Covilakam, Vvk; Klages, Ho; Kleifges, M; Kleinfeller, J; Knapp, F; Kunka, N; Lago, Bl; Langner, N; De Oliveira, Mal; Lenok, ; Letessier-Selvon, A; Lhenry-Yvon, ; Lo Presti, D; Lopes, L; López, R; Lu, L; Luce, Q; Lundquist, Jp; Payeras, Am; Mancarella, G; Mandat, D; Manning, Bc; Manshanden, J; Mantsch, P; Marafico, S; Mariani, Fm; Mariazzi, Ag; Marsella, G; Martello, D; Martinelli, S; Bravo, Om; Mastrodicasa, M; Mathes, Hj; Matthews, J; Matthiae, G; Mayotte, E; Mayotte, S; Mazur, Po; Medina-Tanco, G; Melo, D; Menshikov, A; Michal, S; Micheletti, M; Miramonti, L; Mollerach, S; Montanet, F; Morejon, L; Morello, C; Mostafá, M; Müller, Al; Muller, Ma; Mulrey, K; Mussa, R; Muzio, M; Namasaka, Wm; Nasr-Esfahani, A; Nellen, L; Nicora, G; Niculescu-Oglinzanu, M; Niechciol, M; Nitz, D; Norwood, ; Nosek, D; Novotny, ; Nozka, L; Nucita, A; Núñez, La; Oliveira, C; Palatka, M; Pallotta, J; Papenbreer, P; Parente, G; Parra, A; Pawlowsky, J; Pech, M; Pelayo, R; Peña-Rodriguez, J; Martins, Eep; Armand, Jp; Bertolli, Cp; Perrone, L; Petrera, S; Petrucci, C; Pierog, T; Pimenta, M; Pirronello, ; Platino, M; Pont, B; Pothast, M; Privitera, P; Prouza, M; Puyleart, A; Querchfeld, S; Rautenberg, J; Ravignani, D; Reininghaus, M; Ridky, J; Riehn, F; Risse, M; Rizi, ; De Carvalho, Wr; Rojo, Jr; Roncoroni, Mj; Rossoni, S; Roth, M; Roulet, E; Rovero, Ac; Ruehl, P; Saftoiu, A; Saharan, M; Salamida, F; Salazar, H; Salina, G; Gomez, Jds; Sánchez, F; Santos, Em; Santos, E; Sarazin, F; Sarmento, R; Sarmiento-Cano, C; Sato, R; Savina, P; Schäfer, Cm; Scherini, ; Schieler, H; Schimassek, M; Schimp, M; Schlüter, F; Schmidt, D; Scholten, O; Schoorlemmer, H; Schovánek, P; Schröder, Fg; Schulte, J; Schulz, T; Sciutto, Sj; Scornavacche, M; Segreto, A; Sehgal, S; Shellard, Rc; Sigl, G; Silli, G; Sima, O; Smau, R; Smída, R; Sommers, P; Soriano, Jf; Squartini, R; Stadelmaier, M; Stanca, D; Stasielak, J; Stassi, P; Streich, A; Suárez-Durán, M; Sudholz, T; Suomijärvi, T; Supanitsky, Ad; Szadkowski, Z; Tapia, A; Taricco, C; Timmermans, C; Tkachenko, O; Tobiska, P; Peixoto, Cjt; Tomé, B; Torrès, Z; Travaini, A; Travnicek, P; Trimarelli, C; Tueros, M; Ulrich, R; Unger, M; Vaclavek, L; Vacula, M; Galicia, Jfv; Valore, L; Varela, E; Vásquez-Ramírez, A; Ventura, C; Quispe, Idv; Verzi, V; Vicha, J; Vink, J; Vorobiov, S; Wahlberg, H; Watanabe, C; Watson, Aa; Weindl, A; Wiencke, L; Wittkowski, D; Wundheiler, B; Yushkov, A; Zapparrata, O; Zas, E; Zavrtanik, D; Zavrtanik, M; Zehrer, L. - In: THE ASTROPHYSICAL JOURNAL. - ISSN 0004-637X. - 933:2(2022). [10.3847/1538-4357/ac7393]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1752315
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