Fig. 2
Top: K2 lightcurve for RX J1604.3-2130. Typical uncertainties are smaller than dots. Bottom: Catalina Survey DR2 lightcurve. Since Catalina data cover the epochs of the Spitzer, WISE, and HIRES spectroscopy observations, we have marked them in the figure as vertical lines (see text). In both cases, the average flux (magnitude) is shown as a dotted line.
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