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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 3.

Pattern speed for a toy model in the image domain (shown in warm tones, with color denoting mean brightness at the angular radius, or impact parameter, marked by the top x-axis) and in the (uv) domain (cool tones, with color denoting mean amplitude for a given ρ marked by the bottom x-axis). The image-domain values are measured from an analytic iNoisy model with a known power-law dependence. The best-fit curve to the (uv) pattern speed (blue) asymptotically approaches the brightness-weighted image-domain pattern speed (dashed purple).

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