no code implementations • 23 Sep 2020 • Zhijun Zhao, Haijing Zhou, Yuchen Zhang, Yun Ling, Fangyu Xu
In order to evaluate the ground-based infrared telescope sensitivity affected by the noise from the atmosphere, instruments and detectors, we construct a sensitivity model that can calculate limiting magnitudes and signal-to-noise ratio ($S/N$).
Instrumentation and Methods for Astrophysics