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Event Horizon Telescope Pattern Speeds in the Visibility Domain

  • Authors: Nicholas S. Conroy, Michi Bauböck, Vedant Dhruv, Daeyoung Lee, Chi-kwan Chan, Abhishek V. Joshi, Cora Prather, Charles F. Gammie

Nicholas S. Conroy et al 2026 The Astrophysical Journal 1005 .

  • Provider: AAS Journals

Caption: Figure 5.

Measured (u, v) pattern speeds as a function of baseline length, shown for all SANE face-on models (i = 10∘, 170∘). Color corresponds to the electron temperature distribution function (left) and black hole spin (right). To make the spin dependence clearer, we have not plotted Rhigh = 160 on the right plot. SANE models demonstrate a strong dependence on Rhigh and a weaker dependence on a*.

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