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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 5.

Closure phases on selected triangles at 230 GHz. The solid line (red in the online edition) shows the predicted closure phase in the absence of noise. Each point indicates 10 s of coherently integrated data. The fourth column shows the same triangle as the third column but with a higher data rate and substitution of Chile-10 for Chile-1. The same 2 hr period, corresponding to 4.5 periods (14.8 periods for Model E) is shown in all panels excepting PV-PdB-Chile-10.

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