Paper
1 June 1994 Optimal SNR exposure time for speckle imaging: experimental results with frequency-dependent detector noise
David W. Tyler, Andrew H. Suzuki, Mark A. Von Bokern, Donna D. B. Keating, Michael C. Roggemann
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Abstract
We review recent arguments for using increased spectral bandwidth and exposure times to optimize the signal-to-noise ratio of speckle imaging estimators and discuss the tradeoff between camera exposure time and the number of data frames collected when observing time is fixed. We compare experimental results with a previously-derived expression for optimal exposure time and find reasonable agreement after accounting for frequency-dependent camera noise.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David W. Tyler, Andrew H. Suzuki, Mark A. Von Bokern, Donna D. B. Keating, and Michael C. Roggemann "Optimal SNR exposure time for speckle imaging: experimental results with frequency-dependent detector noise", Proc. SPIE 2198, Instrumentation in Astronomy VIII, (1 June 1994); https://doi.org/10.1117/12.176694
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Cited by 1 scholarly publication.
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KEYWORDS
Signal to noise ratio

Cameras

Spatial frequencies

Speckle imaging

Sensors

Telescopes

Speckle

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