Fig. 5
Top: hard X-ray light curve overlaid with a model of 
ergs s-1 cm-2. Middle: soft X-ray light curve overlaid with a model of 
ergs s-1 cm-2. Bottom: Swift-uvw2 light curve, after subtraction of the galaxy background from a GALEX NUV observation of 2011-05-16, overlaid with a model of 
(solid curve) and a better fitting model of 
(dashed curve).
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