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Super-Resolution Parameter Estimation Using Machine Learning-Assisted Spatial Mode Demultiplexing.

David R Gozzard1,2, John S Wallis1, Alex M Frost1

  • 1International Centre for Radio Astronomy Research, The University of Western Australia, Crawley, WA 6009, Australia.

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|September 13, 2025
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Summary
This summary is machine-generated.

A new machine learning model estimates light source separation below the diffraction limit using spatial mode demultiplexing (SPADE) imaging. This technique offers sub-diffraction resolution for astronomical applications.

Keywords:
machine learningquantum imagingsuper-resolution

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Area of Science:

  • Optics and Photonics
  • Machine Learning Applications
  • Computational Imaging

Background:

  • Resolving fine details in optical imaging is often limited by the diffraction limit.
  • Spatial mode demultiplexing (SPADE) offers a potential pathway to overcome these limitations.
  • Machine learning (ML) presents opportunities for advanced data analysis in complex imaging scenarios.

Purpose of the Study:

  • To develop and evaluate a machine learning model for estimating the separation and relative brightness of closely spaced light sources.
  • To assess the model's performance in achieving sub-diffraction limit resolution.
  • To explore the application of ML-assisted SPADE imaging for overcoming diffraction limitations.

Main Methods:

  • Utilized a multi-planar light converter (MPLC) to perform SPADE imaging.
  • Trained, validated, and tested a lightweight machine learning model on experimental laboratory data.
  • Focused on estimating source separation and relative brightness below the diffraction limit.

Main Results:

  • The ML model accurately estimated source separation up to two orders of magnitude below the diffraction limit for comparable brightness sources.
  • Achieved accurate sub-diffraction separation resolution even when source brightness differed by four orders of magnitude.
  • Performance was limited by cross-talk within the MPLC.

Conclusions:

  • ML-assisted SPADE imaging demonstrates significant potential for achieving sub-diffraction resolution.
  • The developed ML model shows promise for applications in astronomical imaging.
  • Further improvements in MPLC technology could enhance the capabilities of this technique.