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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 7.

A frame from a typical GRMHD model (MAD, a* = 0.5, i = 30, Rhigh = 160) convolved with a 2D Morlet wavelet, showing which image-domain features contribute to the visibility amplitude at ρ = 4 (left), 10 (middle), and 30 (right), filtering for horizontal (top) and vertical features (bottom). The original frame is shown in gray behind the convolution. As expected, large-scale features dominate the low-frequency (uv) data, while small-scale features dominate the high-frequency (uv) data.

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