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
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
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.
Citazione
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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Il report seguente simula gli indicatori relativi alla propria produzione scientifica in relazione alle soglie ASN 2023-2025 del proprio SC/SSD. Si ricorda che il superamento dei valori soglia (almeno 2 su 3) è requisito necessario ma non sufficiente al conseguimento dell'abilitazione. La simulazione si basa sui dati IRIS e sugli indicatori bibliometrici alla data indicata e non tiene conto di eventuali periodi di congedo obbligatorio, che in sede di domanda ASN danno diritto a incrementi percentuali dei valori. La simulazione può differire dall'esito di un’eventuale domanda ASN sia per errori di catalogazione e/o dati mancanti in IRIS, sia per la variabilità dei dati bibliometrici nel tempo. Si consideri che Anvur calcola i valori degli indicatori all'ultima data utile per la presentazione delle domande. La presente simulazione è stata realizzata sulla base delle specifiche raccolte sul tavolo ER del Focus Group IRIS coordinato dall’Università di Modena e Reggio Emilia e delle regole riportate nel DM 589/2018 e allegata Tabella A. Cineca, l’Università di Modena e Reggio Emilia e il Focus Group IRIS non si assumono alcuna responsabilità in merito all’uso che il diretto interessato o terzi faranno della simulazione. Si specifica inoltre che la simulazione contiene calcoli effettuati con dati e algoritmi di pubblico dominio e deve quindi essere considerata come un mero ausilio al calcolo svolgibile manualmente o con strumenti equivalenti.