4.7 Article

Hybrid Very Long Baseline Interferometry Imaging and Modeling withthemis

期刊

ASTROPHYSICAL JOURNAL
卷 898, 期 1, 页码 -

出版社

IOP Publishing Ltd
DOI: 10.3847/1538-4357/ab9c1f

关键词

Black Hole physics; Astronomy data modeling; Computational astronomy; Submillimeter astronomy; Long baseline interferometry; General relativity

资金

  1. Canada Foundation for Innovation (CFI)
  2. ministere de l'Economie, de la science et de l'innovation du Quebec (MESI)
  3. Fonds de recherche du Quebec-Nature et technologies (FRQNT)
  4. Perimeter Institute for Theoretical Physics
  5. Government of Canada through the Department of Innovation, Science and Economic Development Canada
  6. Province of Ontario through the Ministry of Economic Development, Job Creation and Trade
  7. Delaney Family via the Delaney Family John A. Wheeler Chair at Perimeter Institute
  8. Natural Sciences and Engineering Research Council of Canada
  9. ERC synergy grant BlackHoleCam: Imaging the Event Horizon of Black Holes [610058]
  10. Black Hole Initiative at Harvard University - John Templeton Foundation
  11. Gordon and Betty Moore Foundation

向作者/读者索取更多资源

Generating images from very long baseline interferometric observations poses a difficult, and generally not unique, inversion problem. This problem is simplified by the introduction of constraints, some generic (e.g., positivity of the intensity) and others motivated by physical considerations (e.g., smoothness, instrument resolution). It is further complicated by the need to simultaneously address instrumental systematic uncertainties and sparse coverage in theu-vplane. We report a new Bayesian image reconstruction technique in the parameter estimation framework Themisthat has been developed for the Event Horizon Telescope. This has two key features: first, the full Bayesian treatment of the image reconstruction makes it possible to generate a full posterior for the images, permitting a rigorous and quantitative investigation into the statistical significance of image features. Second, it is possible to seamlessly incorporate directly modeled features simultaneously with image reconstruction. We demonstrate this second capability by incorporating a narrow, slashed ring in reconstructions of simulated M87 data in an attempt to detect and characterize the photon ring. We show that it is possible to obtain high-fidelity photon ring sizes, enabling mass measurements with accuracies of 2%-5% that are essentially insensitive to astrophysical uncertainties, and creating opportunities for precision tests of general relativity.

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