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Fig. 3
JHKs photometry of H 1743-322. We show the spectral energy distribution, with reddened magnitudes on the left, and dereddened on the right (corrected from interstellar absorption, see text for details). While the y-axis is offset between the two panels, it has the same scale to better show the effect of the dereddening.
This figure is made of several images, please see below:
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