Theoretical Foundation of Black Hole Image Reconstruction using PRIMO
Dimitrios Psaltis, Feryal Ozel, Lia Medeiros, Tod R. Lauer

TL;DR
This paper provides a theoretical foundation for the PRIMO image-reconstruction algorithm, demonstrating its effectiveness and justification in reconstructing high-resolution black hole images from sparse interferometric data.
Contribution
It offers a theoretical justification for PRIMO's approach, showing it can faithfully reconstruct images using physics-based simulations and a compact set of eigenimages.
Findings
PRIMO achieves native resolution images of the M87 black hole.
The Fourier space smoothing justifies machine learning reconstruction.
PRIMO's eigenimages are compact yet sufficiently complex.
Abstract
A new image-reconstruction algorithm, PRIMO, applied to the interferometric data of the M87 black hole collected with the Event Horizon Telescope (EHT), resulted in an image that reached the native resolution of the telescope array. PRIMO is based on learning a compact set of image building blocks obtained from a large library of high-fidelity, physics-based simulations of black hole images. It uses these building blocks to fill the sparse Fourier coverage of the data that results from the small number of telescopes in the array. In this paper, we show that this approach is readily justified. Since the angular extent of the image of the black hole and of its inner accretion flow is finite, the Fourier space domain is heavily smoothed, with a correlation scale that is at most comparable to the sizes of the data gaps in the coverage of Fourier space with the EHT. Consequently, PRIMO or…
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Taxonomy
TopicsParticle Detector Development and Performance · Medical Imaging Techniques and Applications · Particle physics theoretical and experimental studies
