Comparison of EMCCD post-processing methods for photon counting flux ranges

Nassim Rousset, Jérémie Villeneuve, Jean Hughes Fournier-Lupien, Anis Attiaoui, Gabriel Taillon, Sébastien Francoeur, Olivier Daigle

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Citation (Scopus)

Abstract

Several post-processing methods were proposed to overcome the excess noise factor induced by EMCCD multiplication register. Each method has a unique effect on SNR. However, since SNR does not account for photometric accuracy, it cannot be reliably used to directly compare the performance of these algorithms. A normalized quadratic error that accounts for both SNR and accuracy is proposed as an alternative figure of merit. This approach provides a quantitative and rigorous comparison. Using both experimental and simulated frames in the faint-flux range, it is used to compare the existing EMCCD post-processing methods.

Original languageEnglish
Title of host publicationHigh Energy, Optical, and Infrared Detectors for Astronomy VI
PublisherSPIE
Volume9154
ISBN (Print)9780819496225
DOIs
Publication statusPublished - 2014
Externally publishedYes
EventHigh Energy, Optical, and Infrared Detectors for Astronomy VI - Montreal, QC, Canada
Duration: 2014 Jun 222014 Jun 25

Other

OtherHigh Energy, Optical, and Infrared Detectors for Astronomy VI
CountryCanada
CityMontreal, QC
Period14/6/2214/6/25

    Fingerprint

Keywords

  • Astronomical imaging
  • Bayesian inference
  • EMCCD physics
  • Faint-ux imaging
  • Image post-processing
  • Photodetector figure of merit
  • Photometric accuracy
  • Photon counting

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

Cite this

Rousset, N., Villeneuve, J., Fournier-Lupien, J. H., Attiaoui, A., Taillon, G., Francoeur, S., & Daigle, O. (2014). Comparison of EMCCD post-processing methods for photon counting flux ranges. In High Energy, Optical, and Infrared Detectors for Astronomy VI (Vol. 9154). [91540F] SPIE. https://doi.org/10.1117/12.2055350