Euclid is one of the M-class missions selected for the next phase of ESA’s long-term Cosmic Vision programme. The
primary goal of this mission is to observe the distribution and shapes of distant galaxies, with the aim of mapping and
characterising the dark energy which makes up about 70% of the universe. This will be achieved by measuring the
effects of weak lensing on the captured images, in terms of the distortion caused to the elipticity of galaxy shapes .
The e2v CCD273 was designed for the Euclid mission and is adapted from an older design (the CCD203) with changes
made to improve CTE under irradiation by solar protons. Reducing the effects of radiation damage in the image sensor
will result in images which have minimal distortion.
This paper is focused on the on-going development and verification of 3D device models and their integration with
Monte Carlo radiation damage models. Parameters such as charge interaction volume versus signal size, pixel full well
capacity, and charge transfer behaviour for both the parallel and serial registers will be discussed.
The main mission goals are aimed at measuring distortion due to weak lensing, so it is important to differentiate this
from distortion due to radiation damage. This work will eventually lead to a method of post processing images to remove
the effects of radiation damage.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
A. Clarke ; D. Hall ; N. Murray ; A. Holland and D. Burt
Device modelling and model verification for the Euclid CCD273 detector
", Proc. SPIE 8453, High Energy, Optical, and Infrared Detectors for Astronomy V, 84531I (September 25, 2012); doi:10.1117/12.925887; http://dx.doi.org/10.1117/12.925887