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doit être amélioré et porté à 20 à environ 550 nm pour répondre aux exigences du nouveau projet AMINO (Advanced Multi-spectral Imaging using Novel wavefront sensors with Optical photon-counting detectors
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d'intégration pour l'amplification FI et le multiplexage seront étudiées. Le travail comprendra conception et simulation. Un prototype sera fabriqué. Des tests cryogéniques à 4 K caractériseront les paramètres
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to measure water and carbon monoxide emissions from comets (Microwave Imager for the Rosetta Orbiter-MIRO at 557 GHz); or Jupiter and its Icy moon's atmospheres and surfaces (JUICE-SWI) with two channels
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of the most successful leading physical dissipative process at the origin of FRBs: 'relativistically magnetized shock waves'. In such extreme environments, where magnetic fields routinely reach 10^15 G within a
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into the interstellar medium, not only during supernova explosions but throughout their entire lifetimes. These processes have major consequences for galaxy formation and evolution. Hot stars also exhibit strong
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