All Figures

$\begin{figure} \par\includegraphics[height=10cm,width=8.8cm,clip]{0244fig1.eps} \end{figure}$ Figure 1: Distributions of the deviations of n₁₅ (see text), with respect to $\langle n_{15}\rangle$ , for events of IBD class ( top) and NC class ( middle), and n₁₅ distribution, for CC class ( bottom). The superimposed dashed lines are the fits to zero mean and unit-width Gaussians (IBD and NC) and Poissonian (CC).
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0244fig2.eps} \end{figure}$ Figure 2: Distributions of cluster multiplicities, for IBD class events ( top), NC class ( medium), CC class ( bottom), together with expectations from Poissonian fluctuations, in the case of GW event n.5.
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In the text

$\begin{figure} \par\includegraphics[height=8.8cm,width=8.8cm,clip]{0244fig3.eps} \end{figure}$ Figure 3: Time distribution (bin = 5 s) of the detected pulses (full line for IBD class data and dash-dotted line for NC class data) around the corresponding GW event time (t=0); the bottom panel shows the distribution for the 8 events taken together.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0244fig4.eps} \end{figure}$ Figure 4: $90\%$ c.l. limits to the total energy emitted in neutrinos, in the cooling process, during 20 s, assuming pure Fermi-Dirac spectrum. The dashed line represents the $\rm IH_{\rm ad}$ case, while the other three cases are represented by the solid curve. The limit obtained through NC events is represented by the dash-dotted line.
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In the text

$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0244fig5.eps} \end{figure}$ Figure 5: $90\%$ c.l. limits to the total accretion mass, multiplied by the factor $Y_{\rm n}$ , as a function of $T_{\bar \nu_{\rm e}}$ . The solid line represents the limits obtained using IBD interactions in the case of NH and $\rm IH_{\rm non-ad}$ , the dash-dotted one refers to limit derived through NC events.
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In the text

$\begin{figure} \par\includegraphics[height=10cm,width=8.8cm,clip]{0244fig1.eps} \end{figure}$	Figure 1: Distributions of the deviations of n₁₅ (see text), with respect to $\langle n_{15}\rangle$ , for events of IBD class ( top) and NC class ( middle), and n₁₅ distribution, for CC class ( bottom). The superimposed dashed lines are the fits to zero mean and unit-width Gaussians (IBD and NC) and Poissonian (CC).
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0244fig2.eps} \end{figure}$	Figure 2: Distributions of cluster multiplicities, for IBD class events ( top), NC class ( medium), CC class ( bottom), together with expectations from Poissonian fluctuations, in the case of GW event n.5.
Open with DEXTER

$\begin{figure} \par\includegraphics[height=8.8cm,width=8.8cm,clip]{0244fig3.eps} \end{figure}$	Figure 3: Time distribution (bin = 5 s) of the detected pulses (full line for IBD class data and dash-dotted line for NC class data) around the corresponding GW event time (t=0); the bottom panel shows the distribution for the 8 events taken together.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0244fig4.eps} \end{figure}$	Figure 4: $90\%$ c.l. limits to the total energy emitted in neutrinos, in the cooling process, during 20 s, assuming pure Fermi-Dirac spectrum. The dashed line represents the $\rm IH_{\rm ad}$ case, while the other three cases are represented by the solid curve. The limit obtained through NC events is represented by the dash-dotted line.
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$\begin{figure} \par\includegraphics[width=8.8cm,clip]{0244fig5.eps} \end{figure}$	Figure 5: $90\%$ c.l. limits to the total accretion mass, multiplied by the factor $Y_{\rm n}$ , as a function of $T_{\bar \nu_{\rm e}}$ . The solid line represents the limits obtained using IBD interactions in the case of NH and $\rm IH_{\rm non-ad}$ , the dash-dotted one refers to limit derived through NC events.
Open with DEXTER