\begin{table}%t3 \caption{\label{tab:systematics_gamma}Best-fit transport parameters for different slopes $\gamma$.} %\centering \par \begin{tabular}{lcccccc} \hline\hline\noalign{\smallskip} $\gamma$ & $K_0^{\rm best}\times 10^2$ & $\delta^{\rm best}$ & $V_{\rm c}^{\rm best}$ & $V_{\rm a}^{\rm best}$ & $\chi^2$/d.o.f. \\ & (kpc$^2~$Myr$^{-1}$) & & (km$\;$s$^{-1}$) & (km$\;$s$^{-1}$) & \\\hline & \multicolumn{1}{c}{} \vspace{-0.20cm} \\ 0:~$2.55$ & 4.13 & 0.39 & \dots & \dots & 29.7 \vspace{0.05cm}\\ %chi2=861.177 (31) {\it 0:}~${\it 2.65}$ & {\it 4.08} & {\it 0.40} & {\it \dots}& {\it \dots}& {\it 28.8} \vspace{0.05cm}\\ %chi2=834.898 (31) 0:~$2.75$ & 4.02 & 0.40 & \dots & \dots & 27.9 \vspace{0.05cm}\\ %chi2=809.243 (31) 0:~$2.85$ & 3.97 & 0.40 & \dots & \dots & 27.0 \vspace{0.25cm}\\ %chi2=784.222 (31) % I:~$2.55$ & 0.42 & 0.93 & 14.0 & \dots & 11.4 \vspace{0.05cm}\\ %chi2=317.968 (31) {\it I:}~${\it 2.65}$ & {\it 0.42} & {\it 0.93} & {\it 13.5} & {\it \dots}& {\it 11.2} \vspace{0.05cm}\\ %chi2=313.468 (31) I:~$2.75$ & 0.42 & 0.93 & 13.1 & \dots & 11.0 \vspace{0.05cm}\\ %chi2=308.976 (31) I:~$2.85$ & 0.42 & 0.93 & 12.7 & \dots & 10.9 \vspace{0.25cm}\\ %chi2=304.501 (31) % II:~$2.55$ & 9.41 & 0.24 & \dots & 74.2 & 4.52 \vspace{0.05cm}\\ %chi2=126.547 (31) {\it II:}~${\it 2.65}$ & {\it 9.76} & {\it 0.23} & {\it \dots}& {\it 73.1} & {\it 4.73} \vspace{0.05cm}\\ %chi2=132.498 (31) II:~$2.75$ & 10.1 & 0.23 & \dots & 72.1 & 4.94 \vspace{0.05cm}\\ %chi2=138.361 (31) II:~$2.85$ & 10.4 & 0.22 & \dots & 71.0 & 5.15 \vspace{0.25cm}\\ %chi2=144.132 (31) % III:~$2.55$ & 0.52 & 0.84 & 18.9 & 39.7 & 1.25 \vspace{0.05cm}\\ %chi2=33.8644 (31) {\it III:}~${\it 2.65}$ & {\it 0.48} & {\it 0.86} & {\it 18.8} & {\it 38.0} & {\it 1.47} \vspace{0.05cm}\\ %chi2=39.7024 (31) III:~$2.75$ & 0.45 & 0.87 & 18.8 & 36.4 & 1.75 \vspace{0.05cm}\\ %chi2=47.2764 (31) III:~$2.85$ & 0.42 & 0.88 & 18.6 & 35.0 & 2.10 \vspace{0.10cm}\\ %chi2=56.815 (31) % N.B.: 161 steps between 0.05 and 5000 GeV/n used \hline \end{tabular} \tablefoot{Models 0, I, II, and III for $L=4$~kpc. The parameter $\gamma$ is the slope of the propagated fluxes ($\gamma = \alpha+\delta$). The source spectrum is $Q(E)\propto \beta^{\eta_{\rm S}} {\cal R}^{-\alpha}$, and $\eta_{\rm S}=-1$.} \end{table}