PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.
Scientists are constantly pushing the boundaries, discovering new frontiers of exploration of the Universe; as space missions pursue these challenges it places a greater demand on detector technology advancement. I will present the status of our delta-doped Electron Multiplying CCD (EMCCD) for a UV multi-object spectrograph, the Faint Intergalactic Redshifted Emission Balloon (FB-2). FB-2 demonstrates this new technology, in a low risk suborbital environment, to prove the performance of EMCCDs for future space missions and Technology Readiness Level (TRL) advancement. It uses a new generation controller for counting photons from Nuvucameras. Part of this endeavor will be testing EMCCDs in a radiation environment; initial results will presented in this paper. EMCCDs have proven to be a versatile technology due to its photon counting (PC) capabilities to achieve extremely low readout noise (<< 1 electron). I will present results from the most recent flight and recent noise optimization.
PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.
The alert did not successfully save. Please try again later.
Gillian Kyne, Shouleh Nikzad, April D. Jewell, Samuel Cheng, Todd J. Jones, John Hennessy, Michael Hoenk, "Delta-doped EMCCDs for sub-orbital and space based missions," Proc. SPIE 11454, X-Ray, Optical, and Infrared Detectors for Astronomy IX, 114541I (13 December 2020); https://doi.org/10.1117/12.2561975