Characterization of a photon counting EMCCD for space-based high contrast imaging spectroscopy of extrasolar planets
Ashlee N. Wilkins, Michael W. McElwain, Timothy J. Norton, Bernard J., Rauscher, Johannes F. Rothe, Michael Malatesta, George M. Hilton, James R., Bubeck, Carol A. Grady, Don J. Lindler

TL;DR
This paper discusses the development and characterization of a photon counting EMCCD detector crucial for future space missions aimed at directly imaging and analyzing exoplanets, focusing on overcoming technical challenges like clock-induced charge.
Contribution
It presents progress in characterizing a low-noise EMCCD for space-based exoplanet spectroscopy, including solutions to charge trapping issues, demonstrating its suitability for high-contrast imaging.
Findings
Demonstrated photon counting capability with high gain register
Identified solutions to clock-induced charge problems
Validated detector performance for faint exoplanet signals
Abstract
We present the progress of characterization of a low-noise, photon counting Electron Multiplying Charged Coupled Device (EMCCD) operating in optical wavelengths and demonstrate possible solutions to the problems of Clock-Induced Charge (CIC) and other trapped charge through sub-bandgap illumination. Such a detector will be vital to the feasibility of future space-based direct imaging and spectroscopy missions for exoplanet characterization, and is scheduled to fly on-board the AFTA-WFIRST mission. The 512512 EMCCD is an e2v detector housed and clocked by a N\"uv\"u Cameras controller. Through a multiplication gain register, this detector produces as many as 5000 electrons for a single, incident-photon-induced photoelectron produced in the detector, enabling single photon counting operation with read noise and dark current orders of magnitude below that of standard CCDs. With the…
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