Image Details
Caption: Figure 14.
Relative Bayesian evidence and best-fit mG-ring model diameter vs. m-order, from the snapshot+averaging geometric modeling from the Comrade pipeline applied to the Sgr A* data. Because the absolute values of ﹩\mathrm{ln}{ \mathcal Z }﹩ can be substantially different for each data set (i.e., each combination of observing day, frequency band, and calibration pipeline), and because only the relative values carry information about model specification preferences, we reference all ﹩\mathrm{ln}{ \mathcal Z }﹩ values to the maximum value attained at any m for that data set.
© 2022. The Author(s). Published by the American Astronomical Society.