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Fig. 5.

image

Late-time spectral sequence of iPTF15dtg. All the spectra are absolute-flux calibrated and shown in the rest frame. The zero-flux level for each spectrum is marked by a horizontal dashed line, as well as its phase and telescope. The main SN features are labeled in black at the top, those related to the host-galaxy emission, well visible in the third spectrum, are labeled in red.

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