Spectrally resolved Michelson interferometry. II. Noise analysis
JOSA A, Vol. 18, Issue 3, pp. 614-621 (2001)
http://dx.doi.org/10.1364/JOSAA.18.000614
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Abstract
We study the theoretical noise limitations of a spectrally resolved Michelson interferometer operating in a multispeckle and photon-counting mode. We derive an expression of the signal-to-noise ratio of the fringe modulation in the (cross-) spectral density of short exposures, which allows us to give the signal-to-noise ratio of the various visibility estimators defined in our previous paper [J. Opt. Soc. Am. A 16, 872 (1999)]. These estimators and the corresponding signal-to-noise-ratio expressions are used in the data processing software of the GI2T interferometer in order to estimate the visibility and the accuracy of the measurements.
© 2001 Optical Society of America
[Optical Society of America ]
OCIS Codes
(030.4280) Coherence and statistical optics : Noise in imaging systems
(030.6610) Coherence and statistical optics : Stellar speckle interferometry
Citation
Philippe Berio, D. Mourard, M. Pierron, and A. Chelli, "Spectrally resolved Michelson interferometry. II. Noise analysis," J. Opt. Soc. Am. A 18, 614-621 (2001)
http://www.opticsinfobase.org/josaa/abstract.cfm?URI=josaa-18-3-614
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