Technology advancement of the CCD201-20 EMCCD for the WFIRST coronagraph instrument: sensor characterization and radiation damage
Leon K. Harding, Richard T. Demers, Michael Hoenk, Pavani Peddada,, Bijan Nemati, Michael Cherng, Darren Michaels, Leo S. Neat, Anthony Loc,, Nathan Bush, David Hall, Neil Murray, Jason Gow, Ross Burgon, Andrew Holland,, Alice Reinheimer, Paul R. Jorden, Douglas Jordand

TL;DR
This paper characterizes the CCD201-20 EMCCD sensor for WFIRST's coronagraph, assessing its performance and radiation damage in space-like conditions to ensure low noise imaging for exoplanet detection.
Contribution
It provides the first detailed study of CCD201-20 EMCCD radiation effects under WFIRST-like conditions and evaluates mitigation techniques for space environment damage.
Findings
Radiation damage degrades charge transfer efficiency.
Trap pumping and thermal cycling can mitigate radiation effects.
Sensor characterization confirms suitability for space use.
Abstract
The Wide Field InfraRed Survey Telescope-Astrophysics Focused Telescope Asset (WFIRST-AFTA) mission is a 2.4-m class space telescope that will be used across a swath of astrophysical research domains. JPL will provide a high-contrast imaging coronagraph instrument - one of two major astronomical instruments. In order to achieve the low noise performance required to detect planets under extremely low flux conditions, the electron multiplying charge-coupled device (EMCCD) has been baselined for both of the coronagraph's sensors - the imaging camera and integral field spectrograph. JPL has established an EMCCD test laboratory in order to advance EMCCD maturity to technology readiness level-6. This plan incorporates full sensor characterization, including read noise, dark current, and clock-induced charge. In addition, by considering the unique challenges of the WFIRST space environment,…
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