General relativistic effects and the near-infrared variability of Sgr A* - II. A systematic approach to temporal asymmetry

Open Access

Fig. 3.

Top: one real and three mock light curves. The colored lines show mock light curves generated with the MA model and best-fit posteriors. The black line shows a segment of an observed Sgr A* light curve. Bottom: Kernel functions constructed using τ_1, 2 drawn from the MA-model posterior.

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