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    Correcting photodetector nonlinearity in dual-comb interferometry

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    Type
    Preprint
    Authors
    Guay, Philippe
    Hébert, Nicolas Bourbeau
    Tourigny-Plante, and Alex
    Michaud-Belleau, Vincent
    Genest, Jérôme
    KAUST Grant Number
    OSR-CRG2019-4046
    Date
    2021-08-25
    Preprint Posting Date
    2021-07-05
    Online Publication Date
    2021-08-25
    Print Publication Date
    2021-08-30
    Permanent link to this record
    http://hdl.handle.net/10754/670130
    
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    Abstract
    Photodetector nonlinearity, the main limiting factor in terms of optical power in the detection chain, is corrected to improve the signal-to-noise ratio of a short-time measurement in dual-comb spectroscopy. An iterative correction algorithm minimizing out-of-band spectral artifacts based on nonlinearity correction methods used in classical Fourier-transform spectrometers is presented. The exactitude of the nonlinearity correction is validated using a low power linear measurement. Spectroscopic lines of H$^{12}$CN are provided and the error caused by the saturation of the detector is corrected yielding residuals limited by the measurement noise.
    Citation
    Guay, P., Hébert, N. B., Tourigny-Plante, A., Michaud-Belleau, V., & Genest, J. (2021). Correcting photodetector nonlinearity in dual-comb interferometry. Optics Express, 29(18), 29165. doi:10.1364/oe.435701
    Sponsors
    The authors thank Ian Coddington at NIST for providing the dual-comb system
    Funding. This work was supported by Natural Sciences and Engineering Research Council of Canada (NSERC), Fonds de Recherche du Québec - Nature et Technologies (FRQNT) and the Office of Sponsored Research (OSR) at King Abdullah University of Science and Technology (KAUST) via the Competitive Research Grant (CRG) program with grant # OSR-CRG2019-4046
    Publisher
    arXiv
    DOI
    10.1364/OE.435701
    arXiv
    2107.02138
    Additional Links
    https://arxiv.org/pdf/2107.02138.pdf
    ae974a485f413a2113503eed53cd6c53
    10.1364/OE.435701
    Scopus Count
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