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Fig. 11
Spitzer IRS spectra of NGC 650. Top panel: SL1 spectrum. Bottom panel: combined LL1 and LL2 spectra. The broad feature underneath the [Ne v] 14.3 μm line in the SL1 spectrum is an artifact of the detector, the so-called teardrop. The LL spectra are shown on a logarithmic scale to emphasize the continuum emission.
This figure is made of several images, please see below:
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