Measuring Photon Rings with the ngEHT
Paul Tiede, Michael D. Johnson, Dominic W. Pesce, Daniel C. M., Palumbo, Dominic O. Chang, Peter Galison

TL;DR
This paper assesses the potential of the ngEHT to detect and measure black hole photon rings, highlighting the limitations of current EHT data and the challenges of hybrid imaging techniques in accurately identifying these features.
Contribution
It demonstrates that ngEHT's improved resolution can detect photon rings and critically evaluates the reliability of hybrid imaging methods for their measurement.
Findings
EHT 2017 and 2022 lack sufficient resolution for photon ring detection
ngEHT at 230 GHz and 345 GHz can detect photon rings in models
Hybrid imaging can produce false positives and misinterpret ring properties
Abstract
General relativity predicts that images of optically thin accretion flows around black holes should generically have a ``photon ring,'' composed of a series of increasingly sharp subrings that correspond to increasingly strongly lensed emission near the black hole. Because the effects of lensing are determined by the spacetime curvature, the photon ring provides a pathway to precise measurements of the black hole properties and tests of the Kerr metric. We explore the prospects for detecting and measuring the photon ring using very long baseline interferometry (VLBI) with the Event Horizon Telescope (EHT) and the next generation EHT (ngEHT). We present a series of tests using idealized self-fits to simple geometrical models and show that the EHT observations in 2017 and 2022 lack the angular resolution and sensitivity to detect the photon ring, while the improved coverage and angular…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Pulsars and Gravitational Waves Research · Particle Accelerators and Free-Electron Lasers
