Gregory R. Zengilowskihttps://orcid.org/0000-0002-0515-4813,1 Andre F. Wong,1 Selmer Wong,1 Amy K. Mainzer,1 Sean Careyhttps://orcid.org/0000-0002-0221-6871,2 Ian Diaz Vachier,1 Meghan Dorn,3 Peter R. Eisenhardt,2 Mark Farris,3 Christopher T. Horne,1 Molly Janasik,1 Donald Lee,3 Jessica Maiten,3 Franco Masci,2 Craig McMurtry,4 Jianmei Pan,3 James Peterson,5 Judith Pipher,4 Nick Reilly,4 Lennon Reinhart,5 Michael E. Ressler,2 Kristin Ringhand,4 Jason Surace2
1The Univ. of Arizona (United States) 2California Institute of Technology (United States) 3Teledyne Imaging Sensors (United States) 4Univ. of Rochester (United States) 5Space Dynamics Lab. (United States)
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NEO Surveyor is a NASA Planetary Defense Coordination Office mission designed to detect and track >2/3 of potentially hazardous asteroids >140 m in diameter during its 5-year prime mission. NEO Surveyor entered Phase B in June 2021 and is scheduled to launch in 2026 to survey the sky in two infrared bands. The infrared detectors are a key technology for the mission and have been the subject of focused development for more than a decade. In this paper, we report test results for recently produced detectors and describe design elements of the focal plane module relevant to operations for NEO Surveyor.
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Gregory R. Zengilowski, Andre F. Wong, Selmer Wong, Amy K. Mainzer, Sean Carey, Ian Diaz Vachier, Meghan Dorn, Peter R. Eisenhardt, Mark Farris, Christopher T. Horne, Molly Janasik, Donald Lee, Jessica Maiten, Franco Masci, Craig McMurtry, Jianmei Pan, James Peterson, Judith Pipher, Nick Reilly, Lennon Reinhart, Michael E. Ressler, Kristin Ringhand, Jason Surace, "Status update on the NEO surveyor detector development," Proc. SPIE 12191, X-Ray, Optical, and Infrared Detectors for Astronomy X, 121911V (29 August 2022); https://doi.org/10.1117/12.2629660