Cosmic-Ray Extremely Distributed Observatory

@article{49244,
   author = {Homola, Piotr and Beznosko, Dmitriy and Bhatta, Gopal and Bibrzycki, Lukasz and Borczynska, Michalina and Bratek, Lukasz and Budnev, Nikolay and Burakowski, Dariusz and AlvarezandCastillo, David E. and Almeida Cheminant, Kevin and Cwikla, Aleksander and Damando, Punsiri and Dhital, Niraj and Duffy, Alan R. and Glownia, Piotr and Gorzkiewicz, Krzysztof and Gora, Dariusz and Gupta, Alok C. and Hlavkova, Zuzana and Homola, Martin and Jalocha, Joanna and Kaminski, Robert and Karbowiak, Michal and Kasztelan, Marcin and Kierepko, Renata and Knap, Marek and Kovacs, Peter and Kulinski, Szymon and Lozowski, Bartosz and Magrys, Marek and Medvedev, Mikhail V. and Medrala, Justyna and Mietelski, Jerzy W. and Miszczyk, Justyna and Mozgova, Alona and Napolitano, Antonio and Nazari, Vahab and Ng, Y. Jack and Niedzwiecki, Michal and Oancea, Cristina and Ogan, Boguslaw and Opila, Gabriela and Oziomek, Krzysztof and Pawlik, Maciej and Piekarczyk, Marcin and Poncyljusz, Boezna and Pryga, Jerzy and Rosas, Matias and Rzecki, Krzysztof and ZamoraandSaa, Jilberto and Smelcerz, Katarzyna and Smolek, Karel and Stanek, Weronika and Stasielak, Jaroslaw and Stuglik, Slawomir and Sulma, Jolanta and Sushchov, Oleksandr and Svanidze, Manana and Tam, Kyle M. and Tursunov, Arman and Vaquero, Jose M. and Wibig, Tadeusz and Wozniak, Krzysztof W.},
   article_number = {11},
   doi = {http://dx.doi.org/10.3390/sym12111835},
   keywords = {cosmic rays; cosmic-ray ensembles; extensive air showers; large scale cosmic-ray correlations; CREDO Collaboration},
   language = {eng},
   issn = {2073-8994},
   journal = {Symmetry},
   title = {Cosmic-Ray Extremely Distributed Observatory},
   url = {https://www.mdpi.com/2073-8994/12/11/1835},
   volume = {12},
   year = {2020}
}

TY  - JOUR
ID  - 49244
AU  - Homola, Piotr - Beznosko, Dmitriy - Bhatta, Gopal - Bibrzycki, Lukasz - Borczynska, Michalina - Bratek, Lukasz - Budnev, Nikolay - Burakowski, Dariusz - Alvarez-Castillo, David E. - Almeida Cheminant, Kevin - Cwikla, Aleksander - Dam-o, Punsiri - Dhital, Niraj - Duffy, Alan R. - Glownia, Piotr - Gorzkiewicz, Krzysztof - Gora, Dariusz - Gupta, Alok C. - Hlavkova, Zuzana - Homola, Martin - Jalocha, Joanna - Kaminski, Robert - Karbowiak, Michal - Kasztelan, Marcin - Kierepko, Renata - Knap, Marek - Kovacs, Peter - Kulinski, Szymon - Lozowski, Bartosz - Magrys, Marek - Medvedev, Mikhail V. - Medrala, Justyna - Mietelski, Jerzy W. - Miszczyk, Justyna - Mozgova, Alona - Napolitano, Antonio - Nazari, Vahab - Ng, Y. Jack - Niedzwiecki, Michal - Oancea, Cristina - Ogan, Boguslaw - Opila, Gabriela - Oziomek, Krzysztof - Pawlik, Maciej - Piekarczyk, Marcin - Poncyljusz, Boezna - Pryga, Jerzy - Rosas, Matias - Rzecki, Krzysztof - Zamora-Saa, Jilberto - Smelcerz, Katarzyna - Smolek, Karel - Stanek, Weronika - Stasielak, Jaroslaw - Stuglik, Slawomir - Sulma, Jolanta - Sushchov, Oleksandr - Svanidze, Manana - Tam, Kyle M. - Tursunov, Arman - Vaquero, Jose M. - Wibig, Tadeusz - Wozniak, Krzysztof W.
PY  - 2020
TI  - Cosmic-Ray Extremely Distributed Observatory
JF  - Symmetry
VL  - 12
IS  - 11
SP  - "1835-1"-"1835-55"
EP  - "1835-1"-"1835-55"
SN  - 20738994
KW  - cosmic rays
KW  - cosmic-ray ensembles
KW  - extensive air showers
KW  - large scale cosmic-ray correlations
KW  - CREDO Collaboration
UR  - https://www.mdpi.com/2073-8994/12/11/1835
N2  - The Cosmic-Ray Extremely Distributed Observatory (CREDO) is a newly formed, global collaboration dedicated to observing and studying cosmic rays (CR) and cosmic-ray ensembles (CRE): groups of at least two CR with a common primary interaction vertex or the same parent particle. The CREDO program embraces testing known CR and CRE scenarios, and preparing to observe unexpected physics, it is also suitable for multi-messenger and multi-mission applications. Perfectly matched to CREDO capabilities, CRE could be formed both within classical models (e.g., as products of photon-photon interactions), and exotic scenarios (e.g., as results of decay of Super-Heavy Dark Matter particles). Their fronts might be significantly extended in space and time, and they might include cosmic rays of energies spanning the whole cosmic-ray energy spectrum, with a footprint composed of at least two extensive air showers with correlated arrival directions and arrival times. As the CRE are predominantly expected to be spread over large areas and, due to the expected wide energy range of the contributing particles, such a CRE detection might only be feasible when using all available cosmic-ray infrastructure collectively, i.e., as a globally extended network of detectors. Thus, with this review article, the CREDO Collaboration invites the astroparticle physics community to actively join or to contribute to the research dedicated to CRE and, in particular, to pool together cosmic-ray data to support specific CRE detection strategies.
ER  - 

HOMOLA, Piotr, Dmitriy BEZNOSKO, Gopal BHATTA, Lukasz BIBRZYCKI, Michalina BORCZYNSKA, Lukasz BRATEK, Nikolay BUDNEV, Dariusz BURAKOWSKI, David E. ALVAREZ-CASTILLO, Kevin ALMEIDA CHEMINANT, Aleksander CWIKLA, Punsiri DAM-O, Niraj DHITAL, Alan R. DUFFY, Piotr GLOWNIA, Krzysztof GORZKIEWICZ, Dariusz GORA, Alok C. GUPTA, Zuzana HLAVKOVA, Martin HOMOLA, Joanna JALOCHA, Robert KAMINSKI, Michal KARBOWIAK, Marcin KASZTELAN, Renata KIEREPKO, Marek KNAP, Peter KOVACS, Szymon KULINSKI, Bartosz LOZOWSKI, Marek MAGRYS, Mikhail V. MEDVEDEV, Justyna MEDRALA, Jerzy W. MIETELSKI, Justyna MISZCZYK, Alona MOZGOVA, Antonio NAPOLITANO, Vahab NAZARI, Y. Jack NG, Michal NIEDZWIECKI, Cristina OANCEA, Boguslaw OGAN, Gabriela OPILA, Krzysztof OZIOMEK, Maciej PAWLIK, Marcin PIEKARCZYK, Boezna PONCYLJUSZ, Jerzy PRYGA, Matias ROSAS, Krzysztof RZECKI, Jilberto ZAMORA-SAA, Katarzyna SMELCERZ, Karel SMOLEK, Weronika STANEK, Jaroslaw STASIELAK, Slawomir STUGLIK, Jolanta SULMA, Oleksandr SUSHCHOV, Manana SVANIDZE, Kyle M. TAM, Arman TURSUNOV, Jose M. VAQUERO, Tadeusz WIBIG a Krzysztof W. WOZNIAK. Cosmic-Ray Extremely Distributed Observatory. \textit{Symmetry}. 2020, roč.~12, č.~11, s.~''1835-1''-''1835-55'', 55 s. ISSN~2073-8994. Dostupné z: https://dx.doi.org/10.3390/sym12111835.