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Detecting Flaring Structures in Sagittarius A* with High-Frequency VLBI

  • Authors: Sheperd S. Doeleman, Vincent L. Fish, Avery E. Broderick, Abraham Loeb, and Alan E. E. Rogers

DOELEMAN et al. 2009 The Astrophysical Journal 695 59.

  • Provider: AAS Journals

Caption: Figure 9.

Autocorrelation function plots of selected triangles and quadrangles. Representative models are shown. Black, red, and blue lines indicate ACFs for noiseless data, 16 Gbit s −1, and 4 Gbit s −1, respectively. Panels marked with a red star show ACF ϕ on a different ordinate scale, as indicated to the left in that row; other panels in the same row are on the scale show in the upper left panel. The dotted line shows the period of the hot spot orbit.

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