Andor853:15 Min Direct

The primary challenge identified in the window is the accumulation of dark current.

A integration period is often the "sweet spot" for capturing slow-moving biological processes or faint astronomical nebulae. However, cosmic ray hits increase linearly with time, necessitating robust post-processing algorithms to "clean" the 15-minute frame without losing legitimate signal data. 5. Conclusion andor853:15 min

The use of EM gain effectively reduces read noise to sub-electron levels, making the system ideal for detecting single-photon events during the 15-minute duration. 4. Discussion: The 15-Minute Constraint The primary challenge identified in the window is

A continuous 15-minute integration versus a stacked series of 1-minute exposures. Gain Settings: Varied EM gain levels (1x, 100x, 300x). 3. Noise Analysis and Results 300x). 3. Noise Analysis and Results