Ask any question about EPFL courses, lectures, exercises, research, news, etc. or try the example questions below.
DISCLAIMER: The Graph Chatbot is not programmed to provide explicit or categorical answers to your questions. Rather, it transforms your questions into API requests that are distributed across the various IT services officially administered by EPFL. Its purpose is solely to collect and recommend relevant references to content that you can explore to help you answer your questions.
A new generation of space experiments is needed to enhance our understanding of cosmic rays. The challenge of the direct detection at ever higher energies, with improved energy and angular resolutions, is guiding us in the design of future detectors. The High Energy cosmic-Radiation Detection facility (HERD) onboard the China Space Station will be the next calorimetric experiment. Starting from 2027 and for more than 10 years, HERD will be measuring cosmic protons and heavier nuclei from 30 GeV/nucleon to a few PeV/nucleon. It will search for dark-matter signatures in the energy spectrum of cosmic electrons from 10 GeV to 100 TeV and photons from 100 MeV to 100 TeV. The HERD design, prospects and expected performance, as well as its role in multimessenger astronomy will be presented in this contribution.
Olivier Schneider, Aurelio Bay, Guido Haefeli, Tatsuya Nakada, Frédéric Blanc, Lesya Shchutska, Elena Graverini, Donal Patrick Hill, Marie Theres Christin Bachmayer, Sebastian Schulte, Aravindhan Venkateswaran, Veronica Sølund Kirsebom, Renato Quagliani, Luis Miguel Garcia Martin, Vitalii Lisovskyi, Surapat Ek-In, Serhii Cholak, Federico Ronchetti, Sara Celani, Anni Matilda Kauniskangas, Raphaël van Laak, Ettore Zaffaroni, Elisabeth Maria Niel, Pierre Paul Louis Mayencourt, Brianna Leililani Thielen, Yifei Song, Radoslav Marchevski, Dimitrios Kaminaris
Majed Chergui, Camila Bacellar Cases Da Silveira, Luca Longetti, Ludmila Maria Diniz Leroy, Thomas Roland Barillot