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A Novel Tool for the Absolute End-to-End Calibration of Fluorescence Telescopes – The XY-Scanner

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2024
Autor
Schäfer C.M.; Abdul Halim A.; Abreu P.; Aglietta M.; Allekotte I.; Almeida Cheminant K.; Almela A.; Aloisio R.; Alvarez-Muñiz J.; Ammerman Yebra J.; Anastasi G.A.; Anchordoqui L.; Andrada B.; Andringa S.; Aramo C.; Araújo Ferreira P.R.; Arnone E.; Arteaga Velázquez J.C.; Asorey H.; Assis P.; Avila G.; Avocone E.; Badescu A.M.; Bakalova A.; Balaceanu A.; Barbato F.; Bartz Mocellin A.; Bellido J.A.; Berat C.; Bertaina M.E.; Bhatta G.; Bianciotto M.; Biermann P.L.; Binet V.; Bismark K.; Bister T.; Biteau J.; Blazek J.; Bleve C.; Blümer J.; Boháčová M.; Boncioli D.; Bonifazi C.; Bonneau Arbeletche L.; Borodai N.; Brack J.; Brichetto Orchera P.G.; Briechle F.L.; Bueno A.; Buitink S.; Buscemi M.; Büsken M.; Bwembya A.; Caballero-Mora K.S.; Cabana-Freire S.; Caccianiga L.; Caracas I.; Caruso R.; Castellina A.; Catalani F.; Cataldi G.; Cazon L.; Cerda M.; Cermenati A.; Chinellato J.A.; Chudoba J.; Chytka L.; Clay R.W.; Cobos Cerutti A.C.; Colalillo R.; Coleman A.; Coluccia M.R.; Conceição R.; Condorelli A.; Consolati G.; Conte M.; Convenga F.; Correia dos Santos D.; Costa P.J.; Covault C.E.; Cristinziani M.; Cruz Sanchez C.S.; Dasso S.; Daumiller K.; Dawson B.R.; de Almeida R.M.; de Jesús J.; de Jong S.J.; de Mello Neto J.R.T.; De Mitri I.; de Oliveira J.; de Oliveira Franco D.; de Palma F.; de Souza V.; De Vito E.; Del Popolo A.; Deligny O.; Denner N.; Deval L.; di Matteo A.; Dobre M.; Dobrigkeit C.; D’Olivo J.C.; Domingues Mendes L.M.; dos Anjos J.C.; dos Anjos R.C.; Ebr J.; Ellwanger F.; Emam M.; Engel R.; Epicoco I.; Erdmann M.; Etchegoyen A.; Evoli C.; Falcke H.; Farmer J.; Farrar G.; Fauth A.C.; Fazzini N.; Feldbusch F.; Fenu F.; Fernandes A.; Fick B.; Figueira J.M.; Filipčič A.; Fitoussi T.; Flaggs B.; Fodran T.; Fujii T.; Fuster A.; Galea C.; Galelli C.; García B.; Gaudu C.; Gemmeke H.; Gesualdi F.; Gherghel-Lascu A.; Ghia P.L.; Giaccari U.; Giammarchi M.; Glombitza J.; Gobbi F.; Gollan F.; Golup G.; Gómez Berisso M.; Gómez Vitale P.F.; Gongora J.P.; González J.M.; González N.; Goos I.; Góra D.; Gorgi A.; Gottowik M.; Grubb T.D.; Guarino F.; Guedes G.P.; Guido E.; Hahn S.; Hamal P.; Hampel M.R.; Hansen P.; Harari D.; Harvey V.M.; Haungs A.; Hebbeker T.; Hojvat C.; Hörandel J.R.; Horvath P.; Hrabovský M.; Huege T.; Insolia A.; Isar P.G.; Janecek P.; Johnsen J.A.; Jurysek J.; Kääpä A.; Kampert K.H.; Keilhauer B.; Khakurdikar A.; Kizakke Covilakam V.V.; Klages H.O.; Kleifges M.; Knapp F.; Kunka N.; Lago B.L.; Langner N.; Leigui de Oliveira M.A.; Lema-Capeans Y.; Lenok V.; Letessier-Selvon A.; Lhenry-Yvon I.; Lo Presti D.; Lopes L.; Lu L.; Luce Q.; Lundquist J.P.; Machado Payeras A.; Majercakova M.; Mandat D.; Manning B.C.; Mantsch P.; Marafico S.; Mariani F.M.; Mariazzi A.G.; Mariş I.C.; Marsella G.; Martello D.; Martinelli S.; Martínez Bravo O.; Martins M.A.; Mastrodicasa M.; Mathes H.J.; Matthews J.; Matthiae G.; Mayotte E.; Mayotte S.; Mazur P.O.; Medina-Tanco G.; Meinert J.; Melo D.; Menshikov A.; Merx C.; Michal S.; Micheletti M.I.; Miramonti L.; Mollerach S.; Montanet F.; Morejon L.; Morello C.; Müller A.L.; Mulrey K.; Mussa R.; Muzio M.; Namasaka W.M.; Negi S.; Nellen L.; Nguyen K.; Nicora G.; Niculescu-Oglinzanu M.; Niechciol M.; Nitz D.; Nosek D.; Novotny V.; Nožka L.; Nucita A.; Núñez L.A.; Oliveira C.; Palatka M.; Pallotta J.; Panja S.; Parente G.; Paulsen T.; Pawlowsky J.; Pech M.; Pekala J.; Pelayo R.; Pereira L.A.S.; Pereira Martins E.E.; Perez Armand J.; Pérez Bertolli C.; Perrone L.; Petrera S.; Petrucci C.; Pierog T.; Pimenta M.; Platino M.; Pont B.; Pothast M.; Pourmohammad Shahvar M.; Privitera P.; Prouza M.; Puyleart A.; Querchfeld S.; Rautenberg J.; Ravignani D.; Reininghaus M.; Ridky J.; Riehn F.; Risse M.; Rizi V.; Rodrigues de Carvalho W.; Rodriguez E.; Rodriguez Rojo J.; Roncoroni M.J.; Rossoni S.; Roth M.; Roulet E.; Rovero A.C.; Ruehl P.; Saftoiu A.; Saharan M.; Salamida F.; Salazar H.; Salina G.; Sanabria Gomez J.D.; Sánchez F.; Santos E.M.; Santos E.; Sarazin F.; Sarmento R.; Sato R.; Savina P.; Schäfer C.M.; Scherini V.; Schieler H.; Schimassek M.; Schimp M.; Schlüter F.; Schmidt D.; Scholten O.; Schoorlemmer H.; Schovánek P.; Schröder F.G.; Schulte J.; Schulz T.; Sciutto S.J.; Scornavacche M.; Segreto A.; Sehgal S.; Shivashankara S.U.; Sigl G.; Silli G.; Sima O.; Simon F.; Smau R.; Šmída R.; Sommers P.; Soriano J.F.; Squartini R.; Stadelmaier M.; Stanca D.; Stanič S.; Stasielak J.; Stassi P.; Strähnz S.; Straub M.; Suárez-Durán M.; Suomijärvi T.; Supanitsky A.D.; Svozilikova Z.; Szadkowski Z.; Tapia A.; Taricco C.; Timmermans C.; Tkachenko O.; Tobiska P.; Todero Peixoto C.J.; Tomé B.; Torrès Z.; Travaini A.; Travnicek P.; Trimarelli C.; Tueros M.; Unger M.; Vaclavek L.; Vacula M.; Valdés Galicia J.F.; Valore L.; Varela E.; Vásquez-Ramírez A.; Veberič D.; Ventura C.; Vergara Quispe I.D.; Verzi V.; Vicha J.; Vink J.; Vlastimil J.; Vorobiov S.; Watanabe C.; Watson A.A.; Weindl A.; Wiencke L.; Wilczyński H.; Wittkowski D.; Wundheiler B.; Yue B.; Yushkov A.; Zapparrata O.; Zas E.; Zavrtanik D.; Zavrtanik M.

Citación

       
TY - GEN T1 - A Novel Tool for the Absolute End-to-End Calibration of Fluorescence Telescopes – The XY-Scanner Y1 - 2024 UR - http://hdl.handle.net/11407/8837 PB - et al.; Institute for Cosmic Ray Research (ICRR) Univeristy of Tokyo; International Union of Pure and Applied Physics (IUPAP); JPS; Nagoya Convention and Visitors Bureau; Nagoya University AB - The Pierre Auger Observatory uses 27 large-aperture wide-angle Schmidt telescopes to measure the longitudinal profile of air showers using the air-fluorescence technique. Up to the year 2013, the absolute calibration of the telescopes was performed by mounting a uniform large-diameter light source on each of the telescopes and illuminating the entire aperture with a known photon flux. Due to the high amount of work and person-power required, this procedure was only carried out roughly once every three years, and a relative calibration was performed every night to track short-term changes. Since 2013, only the relative calibration has been performed. In this paper, we present a novel tool for the absolute end-to-end calibration of the fluorescence detectors, the XY-Scanner. The XY-Scanner uses a portable integrating sphere as a light source, which has been absolutely calibrated. This light source is installed onto a motorized rail system and moved across the aperture of each telescope. We mimic the illumination of the entire aperture by flashing the light source at ∼1700 positions evenly distributed across the telescope aperture. For the absolute calibration of the light source, we built a dedicated setup that uses a NIST-calibrated photodiode to measure the average photon flux and a PMT to track the pulse-to-pulse stability. We present the laboratory setups used to study the characteristics of the employed light sources and discuss the inter-calibration between selected telescopes. © Copyright owned by the author(s) under the terms of the Creative Commons. ER - @misc{11407_8837, author = {}, title = {A Novel Tool for the Absolute End-to-End Calibration of Fluorescence Telescopes – The XY-Scanner}, year = {2024}, abstract = {The Pierre Auger Observatory uses 27 large-aperture wide-angle Schmidt telescopes to measure the longitudinal profile of air showers using the air-fluorescence technique. Up to the year 2013, the absolute calibration of the telescopes was performed by mounting a uniform large-diameter light source on each of the telescopes and illuminating the entire aperture with a known photon flux. Due to the high amount of work and person-power required, this procedure was only carried out roughly once every three years, and a relative calibration was performed every night to track short-term changes. Since 2013, only the relative calibration has been performed. In this paper, we present a novel tool for the absolute end-to-end calibration of the fluorescence detectors, the XY-Scanner. The XY-Scanner uses a portable integrating sphere as a light source, which has been absolutely calibrated. This light source is installed onto a motorized rail system and moved across the aperture of each telescope. We mimic the illumination of the entire aperture by flashing the light source at ∼1700 positions evenly distributed across the telescope aperture. For the absolute calibration of the light source, we built a dedicated setup that uses a NIST-calibrated photodiode to measure the average photon flux and a PMT to track the pulse-to-pulse stability. We present the laboratory setups used to study the characteristics of the employed light sources and discuss the inter-calibration between selected telescopes. © Copyright owned by the author(s) under the terms of the Creative Commons.}, url = {http://hdl.handle.net/11407/8837} }RT Generic T1 A Novel Tool for the Absolute End-to-End Calibration of Fluorescence Telescopes – The XY-Scanner YR 2024 LK http://hdl.handle.net/11407/8837 PB et al.; Institute for Cosmic Ray Research (ICRR) Univeristy of Tokyo; International Union of Pure and Applied Physics (IUPAP); JPS; Nagoya Convention and Visitors Bureau; Nagoya University AB The Pierre Auger Observatory uses 27 large-aperture wide-angle Schmidt telescopes to measure the longitudinal profile of air showers using the air-fluorescence technique. Up to the year 2013, the absolute calibration of the telescopes was performed by mounting a uniform large-diameter light source on each of the telescopes and illuminating the entire aperture with a known photon flux. Due to the high amount of work and person-power required, this procedure was only carried out roughly once every three years, and a relative calibration was performed every night to track short-term changes. Since 2013, only the relative calibration has been performed. In this paper, we present a novel tool for the absolute end-to-end calibration of the fluorescence detectors, the XY-Scanner. The XY-Scanner uses a portable integrating sphere as a light source, which has been absolutely calibrated. This light source is installed onto a motorized rail system and moved across the aperture of each telescope. We mimic the illumination of the entire aperture by flashing the light source at ∼1700 positions evenly distributed across the telescope aperture. For the absolute calibration of the light source, we built a dedicated setup that uses a NIST-calibrated photodiode to measure the average photon flux and a PMT to track the pulse-to-pulse stability. We present the laboratory setups used to study the characteristics of the employed light sources and discuss the inter-calibration between selected telescopes. © Copyright owned by the author(s) under the terms of the Creative Commons. OL Spanish (121)
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Resumen
The Pierre Auger Observatory uses 27 large-aperture wide-angle Schmidt telescopes to measure the longitudinal profile of air showers using the air-fluorescence technique. Up to the year 2013, the absolute calibration of the telescopes was performed by mounting a uniform large-diameter light source on each of the telescopes and illuminating the entire aperture with a known photon flux. Due to the high amount of work and person-power required, this procedure was only carried out roughly once every three years, and a relative calibration was performed every night to track short-term changes. Since 2013, only the relative calibration has been performed. In this paper, we present a novel tool for the absolute end-to-end calibration of the fluorescence detectors, the XY-Scanner. The XY-Scanner uses a portable integrating sphere as a light source, which has been absolutely calibrated. This light source is installed onto a motorized rail system and moved across the aperture of each telescope. We mimic the illumination of the entire aperture by flashing the light source at ∼1700 positions evenly distributed across the telescope aperture. For the absolute calibration of the light source, we built a dedicated setup that uses a NIST-calibrated photodiode to measure the average photon flux and a PMT to track the pulse-to-pulse stability. We present the laboratory setups used to study the characteristics of the employed light sources and discuss the inter-calibration between selected telescopes. © Copyright owned by the author(s) under the terms of the Creative Commons.
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http://hdl.handle.net/11407/8837
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Insolia A; Isar P.G; Janecek P; Johnsen J.A; Jurysek J; Kääpä A; Kampert K.H; Karastathis N; Keilhauer B; Kemp J; Khakurdikar A; Kizakke Covilakam V.V; Klages H.O; Kleifges M; Kleinfeller J; Köpke M; Kunka N; Lago B.L; Lang R.G; Langner N; Leigui de Oliveira M.A; Lenok V; Letessier-Selvon A; Lhenry-Yvon I; Lo Presti D; Lopes L; López R; Lu L; Luce Q; Lundquist J.P; Machado Payeras A; Mancarella G; Mandat D; Manning B.C; Manshanden J; Mantsch P; Marafico S; Mariazzi A.G; Mariş I.C; Marsella G; Martello D; Martinelli S; Martínez Bravo O; Mastrodicasa M; Mathes H.J; Matthews J; Matthiae G; Mayotte E; Mazur P.O; Medina-Tanco G; Melo D; Menshikov A; Merenda K.-D; Michal S; Micheletti M.I; Miramonti L; Mollerach S; Montanet F; Morello C; Mostafá M; Müller A.L; Muller M.A; Mulrey K; Mussa R; Muzio M; Namasaka W.M; Nasr-Esfahani A; Nellen L; Niculescu-Oglinzanu M; Niechciol M; Nitz D; Nosek D; Novotny V; Nožka L; Nucita A; Núñez L.A; Palatka M; Pallotta J; Papenbreer P; Parente G; Parra A; Pawlowsky J; Pech M; Pedreira F; Pekala J; Pelayo R; Peña-Rodriguez J; Pereira Martins E.E; Perez Armand J; Pérez Bertolli C; Perlin M; Perrone L; Petrera S; Pierog T; Pimenta M; Pirronello V; 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 V; Rodrigues de Carvalho W; Rodriguez Rojo J; Roncoroni M.J; Rossoni S; Roth M; Roulet E; Rovero A.C; Ruehl P; Saftoiu A; Salamida F; Salazar H; Salina G; Sanabria Gomez J.D; Sánchez F; Santos E.M; Santos E; Sarazin F; Sarmento R; Sarmiento-Cano C; Sato R; Savina P; Schäfer C.M; Scherini V; Schieler H; Schimassek M; Schimp M; Schlüter F; Schmidt D; Scholten O; Schovánek P; Schröder F.G; Schröder S; Schulte J; Sciutto S.J; Scornavacche M; Segreto A; Sehgal S; Shellard R.C; Sigl G; Silli G; Sima O; Šmída R; Sommers P; Soriano J.F; Souchard J; Squartini R; Stadelmaier M; Stanca D; Stanič S; Stasielak J; Stassi P; Streich A; Suárez-Durán M; Sudholz T; Suomijärvi T; Supanitsky A.D; Szadkowski Z; Tapia A; Taricco C; Timmermans C; Tkachenko O; Tobiska P; Todero Peixoto C.J; Tomé B; Torrès Z; Travaini A; Travnicek P; Trimarelli C; Tueros M; Ulrich R; Unger M; Vaclavek L; Vacula M; Valdés Galicia J.F; Valore L; Varela E; Vásquez-Ramírez A; Veberič D; Ventura C; Vergara Quispe I.D; Verzi V; Vicha J; Vink J; Vorobiov S; Wahlberg H; Watanabe C; Watson A.A; Weber M; Weindl A; Wiencke L; Wilczyński H; Wirtz M; Wittkowski D; Wundheiler B; Yushkov A; Zapparrata O; Zas E; Zavrtanik D; Zavrtanik M; Zehrer L; Abbasi R.U; Abu-Zayyad T; Allen M; Arai Y; Arimura R; Barcikowski E; Belz J.W; Bergman D.R; Blake S.A; Buckland I; Cady R; Cheon B.G; Chiba J; Chikawa M; Fujii T; Fujisue K; Fujita K; Fujiwara R; Fukushima M; Fukushima R; Furlich G; Gonzalez R; Hanlon W; Hayashi M; Hayashida N; Hibino K; Higuchi R; Honda K; Ikeda D; Inadomi T; Inoue N; Ishii T; Ito H; Ivanov D; Iwakura H; Iwasaki A; Jeong H.M; Jeong S; Jui C.C.H; Kadota K; Kakimoto F; Kalashev O; Kasahara K; Kasami S; Kawai H; Kawakami S; Kawana S; Kawata K; Kharuk I; Kido E; Kim H.B; Kim J.H; Kim J.H; Kim M.H; Kim S.W; Kimura Y; Kishigami S; Kubota Y; Kurisu S; Kuzmin V; Kuznetsov M; Kwon Y.J; Lee K.H; Lubsandorzhiev B; Lundquist J.P; Machida K; Matsumiya H; Matsuyama T; Matthews J.N; Mayta R; Minamino M; Mukai K; Myers I; Nagataki S; Nakai K; Nakamura R; Nakamura T; Nakamura T; Nakamura Y; Nakazawa A; Nishio E; Nonaka T; Oda H; Ogio S; Ohnishi M; Ohoka H; Oku Y; Okuda T; Omura Y; Ono M; Onogi R; Oshima A; Ozawa S; Park I.H; Potts M; Pshirkov M.S; Remington J; Rodriguez D.C; Rubtsov G.I; Ryu D; Sagawa H; Sahara R; Saito Y; Sakaki N; Sako T; Sakurai N; Sano K; Sato K; Seki T; Sekino K; Shah P.D; Shibasaki Y; Shibata F; Shibata N; Shibata T; Shimodaira H; Shin B.K; Shin H.S; Shinto D; Smith J.D; Sokolsky P; Sone N; Stokes B.T; Stroman T.A; Takagi Y; Takahashi Y; Takamura M; Takeda M; Takeishi R; Taketa A; Takita M; Tameda Y; Tanaka H; Tanaka K; Tanaka M; Tanoue Y; Thomas S.B; Thomson G.B; Tinyakov P; Tkachev I; Tokuno H; Tomida T; Troitsky S; Tsuda R; Tsunesada Y; Uchihori Y; Udo S; Uehama T; Urban F; Wong T; Yada K; Yamamoto M; Yamazaki K; Yang J; Yashiro K; Yoshida F; Yoshioka Y; Zhezher Y; Zundel Z; Pierre Augerc, and the Telescope Arrayd Collaboration (Ciencias BásicasFacultad de Ciencias Básicas, 2022)
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    Auger@TA: An Auger-like surface detector micro-array embedded within the Telescope Array Project 

    Mayotte S.; Caraça-Valente J.; Covault C.; Fujii T.; Im S.; James R.; Johnsen J.; Kampert K.H.; Kern H.; Matthews J.N.; Mayotte E.; Bartz Mocellin A.; Quinn S.; Que H.; Rautenberg J.; Roth M.; Sagawa H.; Sako T.; Sarazin F.; Sato R.; Schmidt D.; Thomas S.B.; Wörner G.; Abdul Halim A.; Abreu P.; Aglietta M.; Allekotte I.; Almeida Cheminant K.; Almela A.; Aloisio R.; Alvarez-Muñiz J.; Ammerman Yebra J.; Anastasi G.A.; Anchordoqui L.; Andrada B.; Andringa S.; Aramo C.; Araújo Ferreira P.R.; Arnone E.; Arteaga Velázquez J.C.; Asorey H.; Assis P.; Avila G.; Avocone E.; Badescu A.M.; Bakalova A.; Balaceanu A.; Barbato F.; Bellido J.A.; Berat C.; Bertaina M.E.; Bhatta G.; Bianciotto M.; Biermann P.L.; Binet V.; Bismark K.; Bister T.; Biteau J.; Blazek J.; Bleve C.; Blümer J.; Bohácová M.; Boncioli D.; Bonifazi C.; Bonneau Arbeletche L.; Borodai N.; Brack J.; Brichetto Orchera P.G.; Briechle F.L.; Bueno A.; Buitink S.; Buscemi M.; Büsken M.; Bwembya A.; Caballero-Mora K.S.; Cabana-Freire S.; Caccianiga L.; Caracas I.; Caruso R.; Castellina A.; Catalani F.; Cataldi G.; Cazon L.; Cerda M.; Cermenati A.; Chinellato J.A.; Chudoba J.; Chytka L.; Clay R.W.; Cobos Cerutti A.C.; Colalillo R.; Coleman A.; Coluccia M.R.; Conceição R.; Condorelli A.; Consolati G.; Conte M.; Convenga F.; Correia dos Santos D.; Costa P.J.; Covault C.E.; Cristinziani M.; Cruz Sanchez C.S.; Dasso S.; Daumiller K.; Dawson B.R.; de Almeida R.M.; de Jesús J.; de Jong S.J.; de Mello Neto J.R.T.; De Mitri I.; de Oliveira J.; de Oliveira Franco D.; de Palma F.; de Souza V.; De Vito E.; Del Popolo A.; Deligny O.; Denner N.; Deval L.; di Matteo A.; Dobre M.; Dobrigkeit C.; D'Olivo J.C.; Domingues Mendes L.M.; dos Anjos J.C.; dos Anjos R.C.; Ebr J.; Ellwanger F.; Emam M.; Engel R.; Epicoco I.; Erdmann M.; Etchegoyen A.; Evoli C.; Falcke H.; Farmer J.; Farrar G.; Fauth A.C.; Fazzini N.; Feldbusch F.; Fenu F.; Fernandes A.; Fick B.; Figueira J.M.; Filipcic A.; Fitoussi T.; Flaggs B.; Fodran T.; Fujii T.; Fuster A.; Galea C.; Galelli C.; García B.; Gaudu C.; Gemmeke H.; Gesualdi F.; Gherghel-Lascu A.; Ghia P.L.; Giaccari U.; Giammarchi M.; Glombitza J.; Gobbi F.; Gollan F.; Golup G.; Gómez Berisso M.; Gómez Vitale P.F.; Gongora J.P.; González J.M.; González N.; Goos I.; Góra D.; Gorgi A.; Gottowik M.; Grubb T.D.; Guarino F.; Guedes G.P.; Guido E.; Hahn S.; Hamal P.; Hampel M.R.; Hansen P.; Harari D.; Harvey V.M.; Haungs A.; Hebbeker T.; Hojvat C.; Hörandel J.R.; Horvath P.; Hrabovský M.; Huege T.; Insolia A.; Isar P.G.; Janecek P.; Johnsen J.A.; Jurysek J.; Kääpä A.; Kampert K.H.; Keilhauer B.; Khakurdikar A.; Kizakke Covilakam V.V.; Klages H.O.; Kleifges M.; Knapp F.; Kunka N.; Lago B.L.; Langner N.; Leigui de Oliveira M.A.; Lema-Capeans Y.; Lenok V.; LetessierSelvon A.; Lhenry-Yvon I.; Lo Presti D.; Lopes L.; Lu L.; Luce Q.; Lundquist J.P.; Machado Payeras A.; Majercakova M.; Mandat D.; Manning B.C.; Mantsch P.; Marafico S.; Mariani F.M.; Mariazzi A.G.; Maris I.C.; Marsella G.; Martello D.; Martinelli S.; Martínez Bravo O.; Martins M.A.; Mastrodicasa M.; Mathes H.J.; Matthews J.; Matthiae G.; Mayotte E.; Mazur P.O.; Medina-Tanco G.; Meinert J.; Melo D.; Menshikov A.; Merx C.; Michal S.; Micheletti M.I.; Miramonti L.; Mollerach S.; Montanet F.; Morejon L.; Morello C.; Müller A.L.; Mulrey K.; Mussa R.; Muzio M.; Namasaka W.M.; Negi S.; Nellen L.; Nguyen K.; Nicora G.; Niculescu-Oglinzanu M.; Niechciol M.; Nitz D.; Nosek D.; Novotny V.; Nožka L.; Nucita A.; Núñez L.A.; Oliveira C.; Palatka M.; Pallotta J.; Panja S.; Parente G.; Paulsen T.; Pawlowsky J.; Pech M.; Pȩkala J.; Pelayo R.; Pereira L.A.S.; Pereira Martins E.E.; Perez Armand J.; Pérez Bertolli C.; Perrone L.; Petrera S.; Petrucci C.; Pierog T.; Pimenta M.; Platino M.; Pont B.; Pothast M.; Pourmohammad Shahvar M.; Privitera P.; Prouza M.; Puyleart A.; Querchfeld S.; Rautenberg J.; Ravignani D.; Reininghaus M.; Ridky J.; Riehn F.; Risse M.; Rizi V.; Rodrigues de Carvalho W.; Rodriguez E.; Rodriguez Rojo J.; Roncoroni M.J.; Rossoni S.; Roth M.; Roulet E.; Rovero A.C.; Ruehl P.; Saftoiu A.; Saharan M.; Salamida F.; Salazar H.; Salina G.; Sanabria Gomez J.D.; Sánchez F.; Santos E.M.; Santos E.; Sarazin F.; Sarmento R.; Sato R.; Savina P.; Schäfer C.M.; Scherini V.; Schieler H.; Schimassek M.; Schimp M.; Schlüter F.; Schmidt D.; Scholten O.; Schoorlemmer H.; Schovánek P.; Schröder F.G.; Schulte J.; Schulz T.; Sciutto S.J.; Scornavacche M.; Segreto A.; Sehgal S.; Shivashankara S.U.; Sigl G.; Silli G.; Sima O.; Simon F.; Smau R.; Šmída R.; Sommers P.; Soriano J.F.; Squartini R.; Stadelmaier M.; Stanca D.; Stanic S.; Stasielak J.; Stassi P.; Strähnz S.; Straub M.; Suárez-Durán M.; Suomijärvi T.; Supanitsky A.D.; Svozilikova Z.; Szadkowski Z.; Tapia A.; Taricco C.; Timmermans C.; Tkachenko O.; Tobiska P.; Todero Peixoto C.J.; Tomé B.; Torrès Z.; Travaini A.; Travnicek P.; Trimarelli C.; Tueros M.; Unger M.; Vaclavek L.; Vacula M.; Valdés Galicia J.F.; Valore L.; Varela E.; Vásquez-Ramírez A.; Veberic D.; Ventura C.; Vergara Quispe I.D.; Verzi V.; Vicha J.; Vink J.; Vlastimil J.; Vorobiov S.; Watanabe C.; Watson A.A.; Weindl A.; Wiencke L.; Wilczynski H.; Wittkowski D.; Wundheiler B.; Yue B.; Yushkov A.; Zapparrata O.; Zas E.; Zavrtanik D.; Zavrtanik M.; Abbasi R.U.; Abe Y.; Abu-Zayyad T.; Allen M.; Arai Y.; Arimura R.; Barcikowski E.; Belz J.W.; Bergman D.R.; Blake S.A.; Buckland I.; Cheon B.G.; Chikawa M.; Fedynitch A.; Fujii T.; Fujisue K.; Fujita K.; Fujiwara R.; Fukushima M.; Furlich G.; Gerber Z.; Globus N.; Hanlon W.; Hayashida N.; He H.; Hibi R.; Hibino K.; Higuchi R.; Honda K.; Ikeda D.; Inoue N.; Ishii T.; Ito H.; Ivanov D.; Iwasaki A.; Jeong H.M.; Jeong S.; Jui C.C.H.; Kadota K.; Kakimoto F.; Kalashev O.; Kasahara K.; Kasami S.; Kawakami S.; Kawata K.; Kharuk I.; Kido E.; Kim H.B.; Kim J.H.; Kim J.H.; Kim S.W.; Kimura Y.; Komae I.; Komori K.; Kusumori Y.; Kuznetsov M.; Kwon Y.J.; Lee K.H.; Lee M.J.; Lubsandorzhiev B.; Lundquist J.P.; Matsuyama T.; Matthews J.A.; Matthews J.N.; Mayta R.; Miyashita K.; Mizuno K.; Mori M.; Murakami M.; Myers I.; Nagataki S.; Nakai K.; Nakamura T.; Nishio E.; Nonaka T.; Ogio S.; Ohoka H.; Okazaki N.; Oku Y.; Okuda T.; Omura Y.; Onishi M.; Ono M.; Oshima A.; Oshima H.; Ozawa S.; Park I.H.; Park K.Y.; Potts M.; Pshirkov M.S.; Remington J.; Rodriguez D.C.; Rott C.; Rubtsov G.I.; Ryu D.; Sagawa H.; Saito R.; Sakaki N.; Sako T.; Sakurai N.; Sato D.; Sato K.; Sato S.; Sekino K.; Shah P.D.; Shibata N.; Shibata T.; Shikita J.; Shimodaira H.; Shin B.K.; Shin H.S.; Shinto D.; Smith J.D.; Sokolsky P.; Stokes B.T.; Stroman T.A.; Takagi Y.; Takahashi K.; Takamura M.; Takeda M.; Takeishi R.; Taketa A.; Takita M.; Tameda Y.; Tanaka K.; Tanaka M.; Thomas S.B.; Thomson G.B.; Tinyakov P.; Tkachev I.; Tokuno H.; Tomida T.; Troitsky S.; Tsuda R.; Tsunesada Y.; Udo S.; Urban F.; Vaiman I.A.; Warren D.; Wong T.; Yamazaki K.; Yashiro K.; Yoshida F.; Zhezher Y.; Zundel Z. (et al.; Institute for Cosmic Ray Research (ICRR) Univeristy of Tokyo; International Union of Pure and Applied Physics (IUPAP); JPS; Nagoya Convention and Visitors Bureau; Nagoya UniversityFacultad de Ciencias Básicas, 2024)
    The Pierre Auger Observatory (Auger) and the Telescope Array Project (TA) are the two largest ultra-highenergy cosmic ray (UHECR) observatories in the world. One obstacle in pursuing full-sky UHECR physics is the apparent ...
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