Des archives aux bases de donnée. Ce programme, propre au Service d'Astrophysique et UMR AIM, comprend l'ensemble des données résultant des programmes d'observations, des projets de simulations ou d'instrumentation. From archives to databases. This research program of the Astrophyscis Division and UMR AIM, consists of all the data resulting from observing programs, simulation projets or instrumentation.
AIM hosts a wide range of research themes developed within thematic teams. All teams are strongly involved in national and international collaborations. Cosmology and Galaxy Evolution (LCEG) The "Cosmology and Galaxy Evolution" team at AIM focuses on studying the formation, evolution, and physical properties of large cosmological structures, galaxy clusters, galaxies themselves, and their internal structures, down to the scales of star formation processes.
Modeling and visualization methods
In preparation
Du calcul à la simulation numérique. Ce programme, propre au Service d'Astrophysique et UMR AIM, comprend l'ensemble des projets en théorie et modélisation. From calculation to numerical simulation. This research program of the Astrophyscis Division and UMR AIM, consists of all the theoretical and modelisation project.
Signal processing and real time systems
Electronic data acquisition systems are used to collect, digitize, format and process data from the detection systems that form the core of experimental physics projects. Irfu laboratories maintain and develop all the hardware, firmware and software skills required to design and implement the entire physical data detection and processing chain.
The AIM instrumentation team oversees the development of cutting-edge spectro-imaging instruments for space missions. Their activities encompass the overall management of instruments, the design and development of systems or subsystems (notably focal planes and their electronics), as well as the assembly, integration, verification, and testing of the developed systems. The team also conducts R&D research, particularly on new detectors.
