Journal
OPTICS EXPRESS
Volume 26, Issue 9, Pages 12049-12056Publisher
OPTICAL SOC AMER
DOI: 10.1364/OE.26.012049
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Funding
- National Science Foundation (NSF) [1256260]
- Intelligence Advanced Research Projects Activity (IARPA) [2016-16041300005]
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The determination of the properties (i.e. line center, width, and amplitude) of a spectral line is simulated using a Monte Carlo method. For dual-comb spectroscopy, ideal repetition rates emerge for both the signal and LO combs that do not correspond to the repetition rates that possess the highest signal-to-noise ratio. The determination is even more accurate when the repetition rates have an arbitrary near-harmonic ratio. The simulation results are generalized to allow for the comparison of any two spectroscopic systems (i.e. not just comb-based systems) by performing the simulations as a function of the spectral point spacing and signal-to-noise ratio of the acquired data. (C) 2018 Optical Society of America under the terms of the OSA Open Access Publishing Agreement
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