Figure 3 from Detecting Flaring Structures in Sagittarius A* with High-Frequency VLBI

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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 3.

Possible ( u, v) tracks for millimeter VLBI. Tracks are labeled by baseline ( A: ALMA/APEX/ASTE, B: Plateau de Bure, C: CARMA, H: Hawaii, L: LMT, S: SMTO, V: Pico Veleta). Unlabelled tracks correspond to the baseline indicated by (− u, − v). Axes are in units of gigawavelengths at ν = 230 GHz.

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