MIRA: A Low-Noise Pixelated ASIC for Photon Counting Applications
摘要
Considering the future long-term space mission programs, many scientific targets will require a payload that includes an UV imager spectrograph. For instance, future missions on gas or ice giant planets will require imaging spectroscopy for a comprehensive study of the aurora footprints and polar magnetosphere as well as the characteristics of the upper atmosphere or exosphere of their satellites