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Fig. 3
IRS spectra of SNe 2003ie, 2004A, 2005ad, and 2006bp. The spectra of SN 2004A are vertically shifted relative to each other by the amount indicated in the label next to the upper spectrum. Strong and wide emission features in the spectrum of SN 2006bp possibly emerge from nearby interstellar clouds.
This figure is made of several images, please see below:
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