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Fig. 2

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Time series of the 150 MHz flux density measured on July 16, 2009, in the direction of the radio source near HAT-P-11. The measurements have been rebinned to 36 min. Triangles and squares correspond to the RR and LL polarizations, respectively. The two vertical long-dashed lines indicate the beginning and the end of the planet’s eclipse behind the host star. The dashed horizontal lines show the box-shaped eclipse light curve fitted to the data points.

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