Author
Zengilowski, G.R.Wong, A.F.
Wong, S.
Mainzer, A.K.
Carey, S.
Vachier, I.D.
Dorn, M.
Eisenhardt, P.R.
Farris, M.
Horne, C.T.
Janasik, M.
Lee, D.
Maiten, J.
Masci, F.
McMurtry, C.
Pan, J.
Peterson, J.
Pipher, J.
Reilly, N.
Reinhart, L.
Ressler, M.E.
Ringhand, K.
Surace, J.
Affiliation
Lunar and Planetary Laboratory, University of ArizonaIssue Date
2022-08-29
Metadata
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SPIECitation
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, and 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/10.1117/12.2629660Rights
© 2022 SPIE.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
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. © 2022 SPIE.Note
Immediate accessISSN
0277-786XVersion
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1117/12.2629660