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A vignetting advantage for thin-film filter arrays in hyperspectral cameras

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arxiv 2003.11983 v1 pith:CIPYFRK7 submitted 2020-03-26 physics.optics astro-ph.IM

classification physics.opticsastro-ph.IM
keywords vignettingspectraladvantagecameracamerasfiltersinterferencesmoothing
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Vignetting in camera lenses is generally seen as something to avoid. For spectral cameras with thin-film interference filters, however, we argue that vignetting can be an advantage. When illuminated by focused light, the bandwidth of interference filters increases with the chief-ray angle, causing position-dependent smoothing of the spectra. We show that vignetting can be used to reduce smoothing and preserve important spectral features. Furthermore, we demonstrate that by adding additional vignetting to a lens, measurements can be made more consistent across the scene. This makes vignetting a useful parameter during spectral camera design.

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  1. Spectral Dual Fitting for $k$-Means

    cs.DS 2026-07 conditional novelty 8.0 of 10

    A spectral dual-fitting algorithm gives (3+ln2+ε)-approximation for Euclidean k-Means and (4.9+ε) for metric k-Means, breaking the metric hardness barrier 1+8/e in Euclidean space.

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