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of the CIGALE software for spatially resolved observations of distant galaxies. The CIGALE software is a global standard for determining the physical parameters of galaxies (stellar mass, star formation rate
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also take part in field surveys to examine the catchment area and observe how particles behave in the stream and pond. In the second stage, the PhD student will examine the particles themselves in
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. However, these test beams can only collect a very small number of neutrinos. This PhD is funded by a joint UChicago-CNRS project entitled "Exploiting Liquid Argon Instruments for sub-GeV Neutrinos" (ELAIN
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are validated on mock-ups and artworks, showcased via AR exhibits at partner museums, and shared openly (data, software, DTs) through European platforms. The Centre for Research and Restoration of the Museums
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the laboratory at the Géosciences Rennes site (Rendal platform); - chronological modelling using software developed in R language. This work will be carried out in close collaboration with other PhD students in
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(LIG), a 450-member laboratory with teaching faculty, full-time researchers, PhD students, administrative and technical staff. The mission of LIG is to contribute to the development of fundamental