Toward a universal characterization methodology for conversion gain measurement of CMOS APS: application to Euclid and SVOM
arXiv:2409.03374 · doi:10.1117/12.3020095
Abstract
With the expanding integration of infrared instruments in astronomical missions, accurate per-pixel flux estimation for near-infrared hybrid detectors has become critical to the success of these missions. Based on CPPM's involvement in both SVOM/Colibri and Euclid missions, this study introduces universally applicable methods and framework for characterizing IR hybrid detectors and decorrelating their intrinsic properties. The characterization framework, applied to the ALFA detector and \Euclid's H2RG, not only validates the proposed methods but also points out subtle behaviors inherent to each detector.
References in corpus (5)
- Euclid. I. Overview of the Euclid mission
- The SVOM Mission
- Properties and characteristics of the WFIRST H4RG-10 detectors
- CAGIRE: a wide-field NIR imager for the COLIBRI 1.3 meter robotic telescope
- Euclid Near Infrared Spectro-Photometer: spatial considerations on H2RG detectors interpixel capacitance and IPC corrected conversion gain from on-ground characterization