English

Deep Learning VLBI Image Reconstruction with Closure Invariants

Instrumentation and Methods for Astrophysics 2024-11-20 v1

Abstract

Interferometric closure invariants, constructed from triangular loops of mixed Fourier components, capture calibration-independent information on source morphology. While a complete set of closure invariants is directly obtainable from measured visibilities, the inverse transformation from closure invariants to the source intensity distribution is not established. In this work, we demonstrate a deep learning approach, Deep learning Image Reconstruction with Closure Terms (DIReCT), to directly reconstruct the image from closure invariants. Trained on both well-defined mathematical shapes (two-dimensional gaussians, disks, ellipses, mm-rings) and natural images (CIFAR-10), the results from our specially designed model are insensitive to station-based corruptions and thermal noise. The median fidelity score between the reconstruction and the blurred ground truth achieved is 0.9\gtrsim 0.9 even for untrained morphologies, where a unit score denotes perfect reconstruction. In our validation tests, DIReCT's results are comparable to other state-of-the-art deconvolution and regularised maximum-likelihood image reconstruction algorithms, with the advantage that DIReCT does not require hand-tuned hyperparameters for each individual prediction. This independent approach shows promising results and offers a calibration-independent constraint on source morphology, ultimately complementing and improving the reliability of sparse VLBI imaging results.

Keywords

Cite

@article{arxiv.2411.12233,
  title  = {Deep Learning VLBI Image Reconstruction with Closure Invariants},
  author = {Samuel Lai and Nithyanandan Thyagarajan and O. Ivy Wong and Foivos Diakogiannis and Lucas Hoefs},
  journal= {arXiv preprint arXiv:2411.12233},
  year   = {2024}
}

Comments

16 pages, 9 figures, submitted to MNRAS

R2 v1 2026-06-28T20:04:34.085Z