English

Automatic Selection of CDS Timing Parameters

Instrumentation and Methods for Astrophysics 2019-07-25 v3

Abstract

CDS is a process used in many CCD readout systems to cancel the reset noise component that would otherwise dominate. CDS processing typically consists of subtracting the integrated video signal during a "signal" period from that during a "reset" period. The response of this processing depends therefore on the shape of the video signal with respect to the integration bounds. In particular, the amount of noise appearing in the final image and the linearity of the pixel value with signal charge are affected by the choice of the CDS timing intervals. In this paper, we use a digital CDS readout system which highly oversamples the video signal (as compared with the pixel rate) to reconstruct pixel values for different CDS timings using identical raw video signal data. We use this technique to develop insights into optimal strategy for selecting CDS timings both in the digital case (where the raw video signal may be available), and in the general case where it is not. In particular, we show that the linearity of the CDS operation allows subtraction of the raw video signals of pixels in bias images from those in illuminated images to directly show the effects of CDS processing on the final (subtracted) pixel values.

Keywords

Cite

@article{arxiv.1902.04125,
  title  = {Automatic Selection of CDS Timing Parameters},
  author = {Daniel P Weatherill and Ian Shipsey and Kirk Arndt and Richard Plackett and Daniel Wood and Kaloyan Metodiev and Maria Mironova and Daniela Bortoletto and Nicolas Demetriou},
  journal= {arXiv preprint arXiv:1902.04125},
  year   = {2019}
}

Comments

presented at Image Sensors for Precision Astronomy (ISPA2018) conference, Caltech, December 2018

R2 v1 2026-06-23T07:38:07.512Z