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Pupil Design for Computational Wavefront Estimation

arXiv 2604.00225 ↗First posted 31 Mar 2026eess.IV cs.CVcited by 0

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Abstract (arXiv)

Establishing a precise connection between imaged intensity and the incident wavefront is essential for emerging applications in adaptive optics, holography, computational microscopy, and non-line-of-sight imaging. While prior work has shown that breaking symmetries in pupil design enables wavefront recovery from a single intensity measurement, there is little guidance on how to design a pupil that improves wavefront estimation. In this work we introduce a quantitative asymmetry metric to bridge this gap and, through an extensive empirical study and supporting analysis, demonstrate that increasing asymmetry enhances wavefront recoverability. We analyze the trade-offs in pupil design, and the impact on light throughput along with performance in noise. Both large-scale simulations and optical bench experiments are carried out to support our findings.

Key facts. No citing papers in the map yet (data through 14 Oct 2026). Builds on 11 of its 52 references that are in the map. First posted on arXiv 31 Mar 2026.

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11 of 52 references.

References · 11

  1. 2015U-Net: Convolutional Networks for Biomedical Image Segmentationcited by 19,713
  2. 2014Phase Retrieval via Wirtinger Flow: Theory and Algorithmscited by 125
  3. 2018prDeep: Robust Phase Retrieval with a Flexible Deep Networkcited by 47
  4. 2013Phase Retrieval from Coded Diffraction Patternscited by 26
  5. 2023On the use of deep learning for phase recoverycited by 20
  6. 2020Solving Phase Retrieval with a Learned Referencecited by 8
  7. 2019Encoding complex fields by using a phase-only optical element: mitigation of pixel crosstalk effectscited by 5
  8. 2024WaveMo: Learning Wavefront Modulations to See Through Scatteringcited by 3
  9. 2025Wavefront Estimation From a Single Measurement: Uniqueness and Algorithmscited by 3
  10. 2025V2V3D: View-to-View Denoised 3D Reconstruction for Light-Field Microscopycited by 2
  11. 2026Guidestar-Free Adaptive Optics with Asymmetric Aperturescited by 2

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