\begin{table}%t2 \caption{\label{t:BAT_XRT_spec}Best-fit model parameters of the 15--150~keV and of the 0.3--10~keV spectra of the $\gamma$-ray prompt and \mbox{X-ray} afterglow measured with BAT and XRT, respectively$^{a}$.} %\centerline {\small \begin{tabular}{lcrrccccc} \hline \hline \noalign{\smallskip} Interval & Energy band & Start time & Stop time & $\beta$ & $N_{\rm H,z}$ & Mean flux & $A_{V,z}^{b}$ & $\chi^2$/d.o.f.\\ & (keV) & (s) & (s) & & ($10^{21}$~cm$^{-2}$) & (erg~cm$^{-2}$~s$^{-1}$) & & \\ \noalign{\smallskip} \hline \noalign{\smallskip} $T_{90}$ & 15--150 & $0.0$ & $67.0$ & $1.44\pm0.46$ & -- & $(3.3\pm0.8)\times10^{-7}$ & -- & $1.44/6$ \\ Total & 15--150 & $-2.0$ & $90.0$ & $1.65\pm0.51$ & -- & $(3.6\pm0.8)\times10^{-7}$ & -- & $5.6/7$ \\ Pulses 1--3 & 15--150 & $-2.0$ & $20.0$ & $2.0\pm0.5$ & -- & $(2.2\pm0.5)\times10^{-7}$ & -- & $1.82/7$ \\ Pulse 4 & 15--150 & $52.9$ & $90.0$ & $1.4\pm0.5$ & -- & $(1.4\pm0.5)\times10^{-7}$ & -- & $5.8/5$ \\ Peak & 15--150 & $0.384$ & $0.832$& $1.1\pm0.6$ & -- & $(1.0\pm0.2)^{c}$ & -- & $6.1/6$ \\ %\hline XRT-WT & 0.3--10 & $77$ & $134$ & $\rm 1.06_{-0.09}^{+0.10}$&$<$1.4& $(4.1\pm0.3)\times10^{-10}$ & -- & $28.3/31$ \\[1mm] Plateau & 0.3--10 & $423$ & $1507$ & $\rm 0.80_{-0.15}^{+0.16}$ & $\rm 1.6_{-1.5}^{+1.8}$ & $(2.3\pm0.3)\times10^{-11}$ & -- & $17.2/24$ \\ %\hline SED~2 & opt-X & $186.8$ & $269.4$ & $0.74\pm0.03$& $[2.7]$ & -- & $<$0.04 & $8.2/6$ \\ SED~3 & opt--X & $423$ & $1507$ & $0.79\pm0.01$ & $2.7\pm0.8$ & -- & $< $0.02 & $32/34$ \\ SED~4 & opt & 78~117 & 93~620 & $0.85\pm0.30$ & -- & -- & $0.10_{-0.06}^{+0.14}$ & $3.4/4$ \\[1mm] %\hline SED~2 & opt & $186.8$ & $269.4$ & $0.61\pm0.13$ & -- & -- & $[0]$ & $3.1/3$ \\ SED~3 & opt & $423$ & $1507$ & $0.74\pm0.05$ & -- & -- & $[0]$ & $7.9/8$ \\ SED~4 & opt & 78~117 & 93~620 & $1.05\pm0.06$ & -- & -- & $[0]$ & $4.8/5$ \\ \hline \end{tabular}} \medskip $^{a}$ The model is an absorbed power law ({\tt xspec} model: {\tt pegpwrlw} for BAT and {\tt wabs} {\tt pow} for XRT data, respectively). Frozen values are reported among square brackets. SED modelling results are also reported, both derived for the broad band from optical to \mbox{X-ray}s and optical points alone. The extinction is modelled with a SMC profile as parametrised by \citet{Pei92}; $^{b}$~rest-frame extinction obtained by modelling the SED with an SMC profile as parametrised by \citet{Pei92}; $^{c}$~peak photon flux in units of ph~cm$^{-2}$~s$^{-1}$. \end{table}