%%%%%%%%%%%%%%%%%%%%%%  Decays  %%%%%%%%%%%%%%%%%%%%%

%D decays
\newcommand{\Dstaunu}      {\mbox{$D_s^{-}\to \tau^{-} \overline{\nu}_{\tau}$}}
\newcommand{\Dstaumu}      {\mbox{$D_s^{-}\to \tau^{-}/\mu \overline{\nu}_{\tau /\mu}$}}
\newcommand{\Dsmunu}      {\mbox{$D_s^{-}\to \mu^{-} \overline{\nu}_{\mu}$}}
\newcommand{\Dsenu}      {\mbox{$D_s^{-}\to \mathrm{e}^{-} \overline{\nu}_{\mathrm{e}}$}}

\newcommand{\Dtaunu}      {\mbox{$D^{+}\to \tau^{+} \nu_{\tau}$}}
\newcommand{\Dmunu}      {\mbox{$D^{+}\to \mu^{+} \nu_{\mu}$}}

\newcommand{\Dkpi}      {\mbox{$\D \to K^{-} \pi^+$}}
\newcommand{\DkpipiO}      {\mbox{$\D \to K^{-} \pi^+ \pi^0$}}
\newcommand{\Dkpipipi}      {\mbox{$\D \to K^{-} \pi^+ \pi^- \pi^+$ }}
\newcommand{\Dkspipi}      {\mbox{$\D \to \overline{K}^{0}_{s} \pi^- \pi^+$}}

\newcommand{\myxDstar}      {\mbox{$D^{*0} \to \D \gamma $}}
\newcommand{\myyDstar}      {\mbox{$D^{*0} \to \D \pi^0 $}}

%%%%%%%%%%%%%%%%%%%%% Efficiencies %%%%%%%%%%%%%%%%%%%%%%

\newcommand{\myeffsig}	   {\mbox{$\epsilon_{\rm sig}$}}
\newcommand{\myefftag}     {\mbox{$\epsilon_{\rm tag}$}}
\newcommand{\myefftot}	   {\mbox{$\epsilon_{\rm tot}$}}
\newcommand{\nsel}         {\mbox{$N_{\rm sel}$}}
\newcommand{\nbg}          {\mbox{$N_{\rm bg}$}}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%



%%%%%%%%%%%%%%%%%%%%% Other %%%%%%%%%%%%%%%%%%%%%%%

\newcommand{\tsp}     {\mbox{\hspace{0.3cm}}}
\newcommand{\etal}      {{\it et~al.}}
\newcommand{\mperiod}      {\mbox{\hspace{0.4cm}.}}

\newcommand{\graphBG}  {Offpeak data and generic Monte Carlo are scaled to onpeak data luminosity}
\newcommand{\graphOFF} {Generic \ccbar, \uds and \tautau Monte Carlo is scaled to offpeak data luminosity}
\newcommand{\graphSIG} {Signal Monte Carlo is scaled to \BR$(\BtoKnunu)  = 5.2 \times 10^{-5}$}

%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
