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First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole

Akiyama, K; Alberdi, A; Alef, W; Asada, K; Azulay, R; Baczko, A-K; Ball, D; ... Yamaguchi, P; + view all (2019) First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole. Astrophysical Journal Letters , 875 (1) , Article L4. 10.3847/2041-8213/ab0e85. Green open access

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Abstract

We present the first Event Horizon Telescope (EHT) images of M87, using observations from April 2017 at 1.3 mm wavelength. These images show a prominent ring with a diameter of ∼40 μas, consistent with the size and shape of the lensed photon orbit encircling the “shadow” of a supermassive black hole. The ring is persistent across four observing nights and shows enhanced brightness in the south. To assess the reliability of these results, we implemented a two-stage imaging procedure. In the first stage, four teams, each blind to the others’ work, produced images of M87 using both an established method (CLEAN) and a newer technique (regularized maximum likelihood). This stage allowed us to avoid shared human bias and to assess common features among independent reconstructions. In the second stage, we reconstructed synthetic data from a large survey of imaging parameters and then compared the results with the corresponding ground truth images. This stage allowed us to select parameters objectively to use when reconstructing images of M87. Across all tests in both stages, the ring diameter and asymmetry remained stable, insensitive to the choice of imaging technique. We describe the EHT imaging procedures, the primary image features in M87, and the dependence of these features on imaging assumptions.

Type: Article
Title: First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole
Open access status: An open access version is available from UCL Discovery
DOI: 10.3847/2041-8213/ab0e85
Publisher version: https://doi.org/10.3847/2041-8213/ab0e85
Language: English
Additional information: Original content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
Keywords: Science & Technology, Physical Sciences, Astronomy & Astrophysics, black hole physics, galaxies: individual (M87), galaxies: jets, techniques: high angular resolution, techniques: image processing, techniques: interferometric, SELF-CALIBRATION, HIGH-RESOLUTION, JET, INTERFEROMETRY, RECONSTRUCTION, IMPLEMENTATION, DECONVOLUTION, PRINCIPLES, MOTION
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/10073505
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