TY - GEN
T1 - Comparison of EMCCD post-processing methods for photon counting flux ranges
AU - Rousset, Nassim
AU - Villeneuve, Jérémie
AU - Fournier-Lupien, Jean Hughes
AU - Attiaoui, Anis
AU - Taillon, Gabriel
AU - Francoeur, Sébastien
AU - Daigle, Olivier
PY - 2014/1/1
Y1 - 2014/1/1
N2 - 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.
AB - 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.
KW - Astronomical imaging
KW - Bayesian inference
KW - EMCCD physics
KW - Faint-ux imaging
KW - Image post-processing
KW - Photodetector figure of merit
KW - Photometric accuracy
KW - Photon counting
UR - http://www.scopus.com/inward/record.url?scp=84906346580&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=84906346580&partnerID=8YFLogxK
U2 - 10.1117/12.2055350
DO - 10.1117/12.2055350
M3 - Conference contribution
AN - SCOPUS:84906346580
SN - 9780819496225
T3 - Proceedings of SPIE - The International Society for Optical Engineering
BT - High Energy, Optical, and Infrared Detectors for Astronomy VI
PB - SPIE
T2 - High Energy, Optical, and Infrared Detectors for Astronomy VI
Y2 - 22 June 2014 through 25 June 2014
ER -