Fig. 7
Second order corrections of two SNe, ID 17135 (SN 2006qm) observed at the NTT (top panel) and ID 17784 (SN 2007jg) observed at the NOT (bottom panel). The observed flux is displayed in black and the corrected flux in light grey. The spectra have been flux calibrated. No corrections due to telluric absorption, Milky Way extinction or effects from host-galaxy light have been applied to the spectra shown here. The inset in each panel shows the relative correction with respect to the observed flux.
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