2020
DOI: 10.1093/imaiai/iaaa023
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Inverting spectrogram measurements via aliased Wigner distribution deconvolution and angular synchronization

Abstract: We propose a two-step approach for reconstructing a signal $\textbf x\in \mathbb{C}^d$ from subsampled discrete short-time Fourier transform magnitude (spectogram) measurements: first, we use an aliased Wigner distribution deconvolution approach to solve for a portion of the rank-one matrix $\widehat{\textbf{x}}\widehat{\textbf{x}}^{*}.$ Secondly, we use angular synchronization to solve for $\widehat{\textbf{x}}$ (and then for $\textbf{x}$ by Fourier inversion). Using this method, we produce two new efficient … Show more

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Cited by 10 publications
(25 citation statements)
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“…We remind the reader that the goal of ptychography is to estimate the a signal y ∈ C d from phaseless measurements through localized masks. A recent method for recovering the signal y from such observation is the BlockPR algorithm by Iwen et al [14], see [9,[22][23][24] for follow-up works developing this algorithm further that also rely on weighted angular synchronization. The BlockPR algorithm proceeds by combining neighboring masks to obtain estimates for the products of entries located close to each other.…”
Section: Improved Error Boundsmentioning
confidence: 99%
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“…We remind the reader that the goal of ptychography is to estimate the a signal y ∈ C d from phaseless measurements through localized masks. A recent method for recovering the signal y from such observation is the BlockPR algorithm by Iwen et al [14], see [9,[22][23][24] for follow-up works developing this algorithm further that also rely on weighted angular synchronization. The BlockPR algorithm proceeds by combining neighboring masks to obtain estimates for the products of entries located close to each other.…”
Section: Improved Error Boundsmentioning
confidence: 99%
“…Combined, they will grant us inequality (18). The first one is required to transit from the signs of z back to z using Inequality (23). The scaling factor guarantees that vector…”
Section: Proof Of Theoremmentioning
confidence: 99%
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“…where x ∈ C d is the sample being imaged, m ∈ C d is a mask which represents the probe's incident illumination on (a portion of) the sample, • denotes the Hadamard (pointwise) product, S k is a shift operator, and D : C d → C d is a function that describes the diffraction of the probe radiation from the sample to the plane of the detector after possibly passing though, e.g, a lens. Prior work in the computational mathematics community related to ptychographic imaging has primarily focused on far-field 1 ptychography (FFP) in which D is the action of a discrete Fourier transform matrix (see, e.g., [10,11,12,13,14,15]) in (1). Here, in contrast, we consider the less well studied setting of near-field ptychography (NFP) which describes situations where the masked sample is too close to the detector to be well described by the FFP model.…”
Section: Introductionmentioning
confidence: 99%