Fig. A.2.
ROSS2 r′ light curve of ISO-ChaI 52 (top panel), ISO-ChaI 35 (middle panel), and Glass L (bottom panel). We have used 2MASS J11042217−7741319 (star 2) for the first two stars and Glass M (star 5) for the latter as comparison stars, adopting the magnitudes listed in Table A.1. The average magnitudes of the last two stars and their rms scatter are provided in the respective panels for the two data segments.
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