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The main goal of the REM project is the observation of prompt afterglow of Gamma-Ray Burst (GRB) events. Such observations at Near InfraRed (NIR) wavelengths are even very promising, since they allow to monitor high-z Ly- absorbed bursts as well as events occurring in dusty star-forming regions. In addition to GRB science, a large amount of time () will be available for different scientific targets: among these the study of variability of stellar objects open exciting new perspectives.

生成讲解博客的中文版本

生成AI智能校验的中文版本