Fig. 13.
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Ratios between the full G-band fluxes and its absorption equivalent widths, the G-band core, and that of nearby Fe I lines. Different seasons of 2016, 2017, and 2018 are marked in red, cyan, and gray. Fitted relations are dotted blue lines, while the identity relations are dashed black. The core flux shows a steeper relative variability than the full band.
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