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Fig. 5


Top: light curve of the 2010 flare component with 30 s exposures and ordinate in mJy (left) and relative flux of the 1995 flare component with 18 min exposures (right). Bottom: blackbody temperature through the 2010 flare (left) and blackbody luminosity (right), derived on the assumption of a time-independent emitting area.

This figure is made of several images, please see below:

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