Speaker
Alberto Gálvez Ureña
Description
Ground-based full-sky studies of the angular distribution of arrival directions of ultra-high-energy cosmic rays require combining data from different observatories, such as the Pierre Auger Observatory (Auger) and the Telescope Array (TA), because no single array can cover all declinations. A working group comprising members from the Auger and TA collaborations has been tasked with performing such studies for more than a decade and has found several indications of full-sky anisotropies. Here, in addition to an overview of previous results, we apply new analysis techniques to data that were previously only used on simulations.
| Collaboration(s) | Pierre Auger and Telescope Array collaborations |
|---|
Authors
Alberto Gálvez Ureña
Luis Anchordoqui
(University of Wisconsin-Milwaukee)
Marta Bianciotto
Peter Biermann
(MPIfR)
Teresa Bister
Jonathan Biteau
(Université Paris-Sud, Université Paris/Saclay, CNRS-IN2P3, Institut de Physique Nucléaire d’Orsay (IPNO), Paris, France)
Lorenzo Caccianiga
(INFN - Sezione di MIlano)
Olivier DELIGNY
Luca Deval
Armando di Matteo
(INFN and University of L'Aquila)
Ugo Gregorio Giaccari
(IMAPP, Radboud University Nijmegen, Nijmegen, The Netherlands)
Geraldina Golup
Ryo Higuchi
Jihyun Kim
(Ulsan National Institute of Science and Technology)
Mikhail Kuznetsov
Jon Paul Lundquist
(University of Nova Gorica - Center for Astrophysics and Cosmology)
FEDERICO MARIA MARIANI
Grigory Rubtsov
(INR RAS)
Peter Tinyakov
(Universite Libre de Bruxelles (ULB))
Federico Urban
(KBFI)
