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5 - 10 July 2026
Copenhagen, Denmark
Conference 14145 > Paper 14145-296
Paper 14145-296

Accurately simulating gain and clock-induced charge production in the EMCCD gain register

9 July 2026 • 17:30 - 19:00 CEST | Room B4-M3

Abstract

An EMCCD will be used for faint companion detection in the Roman Telescope’s coronograph instrument. As the EM gain increases, the chance of clock-induced charge (CIC) production in the gain register increases, which affects the intended multiplication of charge. I have improved the EMCCD detector simulator used for the Roman Telescope, emccd_detect, so that it accounts for this effect. I demonstrate through maximum likelihood estimation that EMCCD data conform better to the modified probability distribution which accounts for this effect. The use of the modified distribution would in principle improve EMCCD calibration and the accuracy of signal extraction from a frame. I discuss the implementation of this as well as other high-gain phenomena in emccd_detect and demonstrate the enhanced accuracy of the simulator.

Presenter

The Univ. of Alabama in Huntsville (United States)
Kevin J. Ludwick is a principal research scientist at the University of Alabama at Huntsville, in the Center for Applied Optics. He does research in image processing, optics calibration, and theoretical cosmology. He earned his PhD in physics at the University of North Carolina and was a Pirrung postdoctoral Fellow at the University of Virginia. He was then a professor at LaGrange College. He has served on the executive committee for the APS FECS.
Presenter/Author
The Univ. of Alabama in Huntsville (United States)