J. Pouthas

TL;DR: The Pierre Auger Observatory as mentioned in this paper, the world's largest cosmic ray observatory, has been in successful operation since completion in 2008 and has recorded data from an exposure exceeding 40,000 km$^2$ sr yr.

TL;DR: The INDRA detector as discussed by the authors is a highly segmented detector for light charged particles and fragments, which covers geometrically 90% of the 4π solid angle and has very low detection thresholds.

TL;DR: The MUST array as discussed by the authors is based on silicon strip technology and dedicated to the study of reactions induced by radioactive beams on light particles, which consists of 8 silicon strip-Si(Li) telescopes used to identify recoiling light charged particles through time of flight, energy loss and energy measurements and to determine precisely their scattering angle through X, Y position measurements.

TL;DR: The INDRA multidetector as discussed by the authors is composed of 96 ionization chambers, 196 silicon detectors, 324 CsI(TI) scintillators and 12 NE102/NE115 phoswich detectors.