Fig. 2

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Optical photometry of V773 Tau system. The four different photometric surveys are represented by different colours, and each photometric series has been normalised using flux outside the main eclipse. The inset panel shows the eclipse light curve in greater detail. The PTF and KELT curves show different depths of the eclipse, indicating the presence of sub-micron dust that causes different amounts of optical extinction in the different pass bands of the two surveys.
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