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End-To-End Deep Neural Network for Salient Object Detection in Complex Environments
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Optical model compression learning for galaxy morphology classification with diffractive deep neural networks.

Zongyu Lu, Jinye Li, Mingxuan Li

    Optics Express
    |June 11, 2026
    PubMed
    Summary
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    Optical computing using diffractive deep neural networks (D2NNs) can analyze galaxy images efficiently. A new optical model compression learning framework improves shallow D2NNs, enhancing galaxy classification accuracy and robustness for astronomical data analysis.

    Area of Science:

    • Astronomy and Astrophysics
    • Computer Science
    • Optical Computing

    Background:

    • Galaxy morphology is crucial for understanding cosmic evolution.
    • Large astronomical surveys generate vast datasets, posing challenges for energy-efficient processing.
    • Diffractive deep neural networks (D2NNs) offer high-throughput, low-power optical computing but face limitations with depth (attenuation) and shallow networks (representation).

    Purpose of the Study:

    • To address the trade-off between depth and representation in D2NNs for astronomical data analysis.
    • To develop an optical model compression learning (OMCL) framework for D2NNs.
    • To improve the performance and practicality of optical neural networks for large-scale galaxy surveys.

    Main Methods:

    • Extended knowledge distillation with optical-domain considerations to create the OMCL framework.

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  • Applied OMCL to compress deep D2NNs into shallower models.
  • Conducted numerical simulations using galaxy images from the Sloan Digital Sky Survey (SDSS).
  • Main Results:

    • The compressed D2NN model achieved 69.25% classification accuracy on SDSS galaxy images, a 27.5% improvement over conventional training.
    • The model demonstrated partial recognition of unseen galaxy categories.
    • Compressed models exhibited smoother, sparser phase patterns, enhancing noise robustness and tolerance to low-precision quantization (3-bit).

    Conclusions:

    • Transferring optical-domain features from deeper networks effectively mitigates limitations in shallow D2NNs.
    • The OMCL framework provides a practical approach for developing fabrication-friendly, high-performance optical neural networks.
    • This research paves the way for efficient optical analysis of large astronomical datasets.