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Ground observations of a space laser for the assessment of its in-orbit performance
The Pierre Auger Collaboration, O. Lux, I. Krisch +380
The wind mission Aeolus of the European Space Agency was a groundbreaking achievement for Earth observation. Between 2018 and 2023, the space-borne lidar instrument ALADIN onboard…
Shore Shadow Effect in Baikal
Apoorva Bhatta, Paweł Malecki, Dariusz Góra
The measurement of the individual charged particles especially muons in an extended air shower (EAS) resulting from primary cosmic rays provides important distinguishing parameters…
The FRAM robotic telescope for atmospheric monitoring at the Pierre Auger Observatory
The Pierre Auger Collaboration, A. Aab, P. Abreu +377
FRAM (F/Photometric Robotic Atmospheric Monitor) is a robotic telescope operated at the Pierre Auger Observatory in Argentina for the purposes of atmospheric monitoring using stell…
Calibration of the underground muon detector of the Pierre Auger Observatory
The Pierre Auger Collaboration, A. Aab, P. Abreu +370
To obtain direct measurements of the muon content of extensive air showers with energy above eV, the Pierre Auger Observatory is currently being equipped with an underg…
Design, upgrade and characterization of the silicon photomultiplier front-end for the AMIGA detector at the Pierre Auger Observatory
The Pierre Auger Collaboration, A. Aab, P. Abreu +357
AMIGA (Auger Muons and Infill for the Ground Array) is an upgrade of the Pierre Auger Observatory to complement the study of ultra-high-energy cosmic rays (UHECR) by measuring the…
Recognition and classification of the cosmic-ray events in images captured by CMOS/CCD cameras
Michal Niedzwiecki, Krzysztof Rzecki, Marta Marek +15
Muons and other ionizing radiation produced by cosmic rays and radiative decays affect CMOS/CCD sensor. When particles colliding with sensors atoms cause specific kind of noise on…
A communication solution for portable detectors of the Cosmic Ray Extremely Distributed Observatory
Katarzyna Smelcerz, Konrad Kopański, Wojciech Noga +17
The search for Cosmic-Ray Ensembles (CRE), groups of correlated cosmic rays that might be distributed over very large areas, even of the size of the planet, requires a globally spr…
Search for ultra-high energy photons: observing the preshower effect with gamma-ray telescopes
Kevin Almeida Cheminant, Dariusz Gora, David E. Alvarez Castillo +16
Ultra-high energy photons constitute one of the most important pieces of the astroparticle physics problems. Their observation may provide new insight on several phenomena such as…
The Pierre Auger Observatory: review of latest results and perspectives
Dariusz Gora
The Pierre Auger Observatory is the world's largest operating detection system for the observation of ultra high energy cosmic rays (UHECRs). The detector allows detailed measureme…
Search for tau neutrinos at PeV energies and beyond with the MAGIC telescopes
D. Gora, M. Manganaro, E. Bernardini +5
The MAGIC telescopes, located at the Roque de los Muchachos Observatory (2200 a.s.l.) in the Canary Island of La Palma, are placed on the top of a mountain, from where a window of…
Cosmic-Ray Extremely Distributed Observatory: a global cosmic ray detection framework
O. Sushchov, P. Homola, N. Dhital +19
The main objective of the Cosmic-Ray Extremely Distributed Observatory (CREDO) is the detection and analysis of extended cosmic ray phenomena, so-called super-preshowers (SPS), usi…
We are all the Cosmic-Ray Extremely Distributed Observatory
N. Dhital, P. Homola, J. F. Jarvis +22
The Cosmic-Ray Extremely Distributed Observatory (CREDO) is an infrastructure for global analysis of extremely extended cosmic-ray phenomena, so-called super-preshowers, beyond the…
Search for electromagnetic super-preshowers using gamma-ray telescopes
K. Almeida Cheminant, D. Gora, N. Dhital +22
Any considerations on propagation of particles through the Universe must involve particle interactions: processes leading to production of particle cascades. While one expects exis…
Performance of the MAGIC telescopes under moonlight
D. Guberman, P. Colin
MAGIC, a system of two imaging atmospheric Cherenkov telescopes, achieves its best performance under dark conditions, i.e. in absence of moonlight or twilight. Since operating the…
Performance of the MAGIC telescopes under moonlight
MAGIC Collaboration, M. L. Ahnen, S. Ansoldi +143
MAGIC, a system of two imaging atmospheric Cherenkov telescopes, achieves its best performance under dark conditions, i.e. in absence of moonlight or twilight. Since operating the…
Detection of tau neutrinos by Imaging Air Cherenkov Telescopes
Dariusz Gora, Elisa Bernardini
This paper investigates the potential to detect tau neutrinos in the energy range of 1-1000 PeV searching for very inclined showers with imaging Cherenkov telescopes. A neutrino in…
IceCube-Gen2 - The Next Generation Neutrino Observatory at the South Pole: Contributions to ICRC 2015
Gen2 Collaboration, M. G. Aartsen, K. Abraham +337
Papers submitted to the 34th International Cosmic Ray Conference (ICRC 2015, The Hague) by the IceCube-Gen2 Collaboration.
Detection of tau neutrinos by Imaging Air Cherenkov Telescopes
Dariusz Gora, Elisa Bernardini
This paper investigates the potential to detect tau neutrinos in the energy range of 1-1000 PeV searching for very inclined showers with imaging Cherenkov telescopes. A neutrino in…
Searching for tau neutrinos with Cherenkov telescopes
D. Gora, E. Bernardini, A. Kappes
Cherenkov telescopes have the capability of detecting high energy tau neutrinos in the energy range of 1--1000 PeV by searching for very inclined showers. If a tau lepton, produced…
Improvement in Fast Particle Track Reconstruction with Robust Statistics
M. G. Aartsen, R. Abbasi, Y. Abdou +277
The IceCube project has transformed one cubic kilometer of deep natural Antarctic ice into a Cherenkov detector. Muon neutrinos are detected and their direction inferred by mapping…
Measurement of South Pole ice transparency with the IceCube LED calibration system
IceCube Collaboration, M. G. Aartsen, R. Abbasi +272
The IceCube Neutrino Observatory, approximately 1 km^3 in size, is now complete with 86 strings deployed in the Antarctic ice. IceCube detects the Cherenkov radiation emitted by ch…
IceTop: The surface component of IceCube
IceCube Collaboration, R. Abbasi, Y. Abdou +280
IceTop, the surface component of the IceCube Neutrino Observatory at the South Pole, is an air shower array with an area of 1 km2. The detector allows a detailed exploration of the…
Trigger and Aperture of the Surface Detector Array of the Pierre Auger Observatory
J. Abraham, P. Abreu, M. Aglietta +469
The surface detector array of the Pierre Auger Observatory consists of 1600 water-Cherenkov detectors, for the study of extensive air showers (EAS) generated by ultra-high-energy c…
The Design and Performance of IceCube DeepCore
The IceCube Collaboration
The IceCube neutrino observatory in operation at the South Pole, Antarctica, comprises three distinct components: a large buried array for ultrahigh energy neutrino detection, a su…