Paper 14145-146
CuRIOS-ED: optical AIT workflow and on-ground performance characterization of a 12U CubeSat imaging payload
6 July 2026 • 17:30 - 19:00 CEST | Room B4-M3
Abstract
CuRIOS-ED (CubeSats for Rapid Infrared and Optical Surveys – Exploration Demo) is a 12U CubeSat payload and pathfinder for the CuRIOS constellation, a fleet of CubeSats for optical monitoring of the transient sky. The payload combines a commercial Simera f/6 telescope with a Sony IMX455 CMOS detector in a custom camera housing. The system delivers a 3° field of view. We present the optical AIT workflow and on-ground performance of the telescope–detector assembly. A metrology-based alignment scheme positions the focal plane within the ±50 µm depth of focus, with a mean focus error <5 µm across the 36×24 mm sensor. End-to-end tests on a clean-room bench, using a custom OAP collimator, yield PSFs with core FWHM ≲1 pixel (<1.5″), consistent with the vendor wavefront map. PSF mapping after qualification-level vibration shows no measurable degradation, indicating that the CuRIOS-ED optical payload meets its image-quality budget and is robust against launch loads.
Presenter
Univ. of California, Berkeley (United States)
Dr. Charles-Antoine Claveau joined Prof. Jessica Lu’s MULab at UC Berkeley as a postdoctoral researcher in late 2023. He is currently working on the design of the CuRIOS space project, including the AIT activities for the CuRIOS-ED demonstrator; on the astrometric calibration of the Keck telescopes; and on detector characterization for the VisMCAO concept on Keck. This work is part of the MULab’s microlensing survey to detect stellar-mass black holes.
He was previously a postdoctoral researcher in Prof. Michael Bottom’s group at the Institute for Astronomy in Hawaii, starting in 2020, where he worked on developing the next generation of LmAPD detectors dedicated to very-low-background infrared astronomy. He completed his PhD in cosmology in 2019 at the University of Paris-Saclay, with a dissertation on the construction of the spectrographs and quasar target selection for the Dark Energy Spectroscopic Instrument (DESI) project.