Gaia serial CTI modelling and radiation damage study
C. Pagani, N. C. Hambly, M. Davidson, N. Rowell, C. Crowley, R. Collins, F. van Leeuwen, G. M. Seabroke, A. Holland, M. A. Barstow, and D. W. Evans

TL;DR
This paper presents a detailed, physically motivated model for CCD radiation damage in Gaia's spacecraft, focusing on serial CTI effects, calibrated with mission data to improve astrometric accuracy.
Contribution
It introduces CtiPixel, a pixel-based CTI model for Gaia CCDs, calibrated with serial CTI diagnostics, revealing damage evolution and defect characteristics over the mission.
Findings
Serial CTI increases slowly over time with sudden jumps after solar events.
The model accurately reproduces observed CTI signatures in calibration data.
Damage evolution correlates with space weather and CCD annealing procedures.
Abstract
During the course of its mission, ESA's Gaia spacecraft has generated a map of the stars of the Galaxy of exquisite detail. While in its L2 orbit, the satellite has been exposed to high energy cosmic rays and solar particles, that caused permanent damage to its CCDs. The main effect of radiation damage on Gaia data is the distortion of its images and spectra, caused by the CCDs charge transfer inefficiency (CTI) during the readout process, that, if not taken into account, can result in inaccurate measurements of a star's location and flux. In this work, the impact of CTI in the serial readout direction, larger than in the parallel due to the presence of CCDs manufacturing defects, has been analysed and modelled. A pixel-based, physically motivated CTI model, CtiPixel, has been developed to characterise the damage in Gaia CCDs. The model has been calibrated using dedicated serial CTI…
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Taxonomy
TopicsCCD and CMOS Imaging Sensors · Gamma-ray bursts and supernovae · Solar and Space Plasma Dynamics
