Bayesian fitting to mock GRAVITY data shows robust detection of secondary images from Sgr A* flares requires both an order-of-magnitude larger sample and astrometric uncertainties reduced to 40% of current levels for |ΔBIC| > 7.9.
The Physical Origin and TimeLagofMultifrequencyFlaresfromSgrA*
2 Pith papers cite this work. Polarity classification is still indexing.
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