$\begin{figure} \par\includegraphics[angle=-90,width=7.6cm,clip]{0675fig1a.eps}\p... ...e*{2mm} \includegraphics[angle=-90,width=7.6cm,clip]{0675fig1b.eps} \end{figure}$ Figure 1: Inverse wavelet reconstruction of separate scales of the wavelet decomposition of a spectrum of SN 1994D. The sum of contributions from scales 7-14 is used to construct the wavelet transformed spectra, $F_{w}(\lambda )$ , used in this work.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7cm,clip]{0675fig2.eps} \end{figure}$ Figure 2: Illustration of the $EW_{w}\{{\rm Si}~{\rm II}\}$ definition on a wavelet transformed spectrum, $F_{w}(\lambda )$ , of SN 1994D.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{0675fig3.eps} \end{figure}$ Figure 3: Relative error of the measured $EW_{w}\{{\rm Si}~{\rm II}\}$ as a function of q, the amount of host contamination for elliptical (open symbols) and spiral (filled symbols) galaxies for 3 low-z SNe, 1981B, 1994D and 2002bo (given as triangle, diamond and square symbols respectively).
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{0675fig4a.eps}\p... ...e*{2mm} \includegraphics[angle=-90,width=7.5cm,clip]{0675fig4b.eps} \end{figure}$ Figure 4: $EW_{w}\{{\rm Si}~{\rm II}\}$ versus x₁ ( top) and colour ( bottom) estimated using SALT2 including high-z SNe. The colours chosen for different sub-classes are the same as in Benetti et al. (2005); Pastorello et al. (2007b): blue filled squares for HVG SNe, light green filled circles for LVG SNe and red symbols for FAINT SNe.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{0675fig5.eps} \end{figure}$ Figure 5: Morphological type of the SN host galaxy versus measured $EW_{w}\{{\rm Si}~{\rm II}\}$ for nearby SNe.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=7.6cm,clip]{0675fig1a.eps}\p... ...e*{2mm} \includegraphics[angle=-90,width=7.6cm,clip]{0675fig1b.eps} \end{figure}$	Figure 1: Inverse wavelet reconstruction of separate scales of the wavelet decomposition of a spectrum of SN 1994D. The sum of contributions from scales 7-14 is used to construct the wavelet transformed spectra, $F_{w}(\lambda )$ , used in this work.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=-90,width=7cm,clip]{0675fig2.eps} \end{figure}$	Figure 2: Illustration of the $EW_{w}\{{\rm Si}~{\rm II}\}$ definition on a wavelet transformed spectrum, $F_{w}(\lambda )$ , of SN 1994D.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{0675fig3.eps} \end{figure}$	Figure 3: Relative error of the measured $EW_{w}\{{\rm Si}~{\rm II}\}$ as a function of q, the amount of host contamination for elliptical (open symbols) and spiral (filled symbols) galaxies for 3 low-z SNe, 1981B, 1994D and 2002bo (given as triangle, diamond and square symbols respectively).
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{0675fig4a.eps}\p... ...e*{2mm} \includegraphics[angle=-90,width=7.5cm,clip]{0675fig4b.eps} \end{figure}$	Figure 4: $EW_{w}\{{\rm Si}~{\rm II}\}$ versus x₁ ( top) and colour ( bottom) estimated using SALT2 including high-z SNe. The colours chosen for different sub-classes are the same as in Benetti et al. (2005); Pastorello et al. (2007b): blue filled squares for HVG SNe, light green filled circles for LVG SNe and red symbols for FAINT SNe.
Open with DEXTER

$\begin{figure} \par\includegraphics[angle=-90,width=7.5cm,clip]{0675fig5.eps} \end{figure}$	Figure 5: Morphological type of the SN host galaxy versus measured $EW_{w}\{{\rm Si}~{\rm II}\}$ for nearby SNe.
Open with DEXTER