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- FZU ‒ Institute of Physics of the Academy of Sciences of the Czech RepublicCZ325 papers
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12 papers · 1 filter
Developments and results in the context of the JEM-EUSO program obtained with the ESAF Simulation and Analysis Framework
S. Abe, J. H. Adams, D. Allard +172
JEM--EUSO is an international program for the development of space-based Ultra-High Energy Cosmic Ray observatories. The program consists of a series of missions which are either u…
Periodic patterns for resolution limit characterization of correlation plenoptic imaging
Francesco Scattarella, Gianlorenzo Massaro, Bohumil Stoklasa +2
The measurement of the spatio-temporal correlations of light provides an interesting tool to overcome the traditional limitations of standard imaging, such as the strong trade-off…
Reconstruction procedure of the Fluorescence detector Array of Single-pixel Telescopes (FAST)
Fraser Bradfield, Justin Albury, Jose Bellido +31
The Fluorescence detector Array of Single-pixel Telescopes (FAST) is one of several proposed designs for a next-generation cosmic-ray detector. Such detectors will require enormous…
Detecting ultra-high-energy cosmic rays with prototypes of the Fluorescence detector Array of Single-pixel Telescopes (FAST) in both hemispheres
Shunsuke Sakurai, Justin Albury, Jose Bellido +31
Ultra-high energy cosmic rays (UHECRs), whose energy are beyond , are the most energetic particles we have ever detected. The latest results seem to indicate a…
Selective Activation of Aromatic C-H Bonds Catalyzed by Single Gold Atoms at Room Temperature
Benjamin Lowe, Jack Hellerstedt, Adam Matěj +5
Selective activation and controlled functionalization of C-H bonds in organic molecules is one of the most desirable processes in synthetic chemistry. Despite progress in heterogen…
Search for UHE Photons from Gravitational Wave Sources with the Pierre Auger Observatory
The Pierre Auger Collaboration, A. Abdul Halim, P. Abreu +368
A search for time-directional coincidences of ultra-high-energy (UHE) photons above 10 EeV with gravitational wave (GW) events from the LIGO/Virgo runs O1 to O3 is conducted with t…