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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 4.

Measured (u, v) pattern speeds as a function of baseline length, shown for all MAD face-on models (i = 10∘, 170∘). Color corresponds to dimensionless black hole spin a*. Notice that prograde (a* > 0) models slope more steeply, while retrograde (a* < 0) models have a shallower slope.

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