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commands.tex
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commands.tex
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\usepackage{xspace}
\usepackage{color}
\usepackage{xcolor}
\usepackage{rotating}
\definecolor{light-gray}{gray}{0.8}
%\newcommand{\jpsi}{\rm J/$\psi$}
%\newcommand{\psip}{$\psi^\prime$}
%\newcommand{\jpsiDY}{\rm J/$\psi$\,/\,DY}
%\newcommand{\dd}{\mathrm{d}}
%\newcommand{\chic}{$\chi_{\rm c}$}
%\newcommand{\ezdc}{$E_{\rm ZDC}$}
%\newcommand{\red}{\textcolor{red}}
%\newcommand{\blue}{\textcolor{blue}}
\newcommand{\pp}{\ensuremath{\rm pp}\xspace}
\newcommand{\pPb}{p--Pb\xspace}
\newcommand{\PbPb}{Pb--Pb\xspace}
\newcommand{\AuAu}{Au--Au\xspace}
\newcommand{\ppbar}{\ensuremath{\rm p\bar{p}}\xspace}
\newcommand{\epluseminus}{\ensuremath{\rm e^{+}e^{-}}\xspace}
\newcommand{\ep}{\ensuremath{\rm ep}\xspace}
\newcommand{\MeVc}{\ensuremath{{\rm MeV/}c}\xspace}
\newcommand{\MeVcsq}{\ensuremath{{\rm MeV/}c^{2}}\xspace}
\newcommand{\GeVc}{\ensuremath{{\rm GeV/}c}\xspace}
\newcommand{\GeVcsq}{\ensuremath{{\rm GeV/}c^{2}}\xspace}
\newcommand{\eV}{\ensuremath{\rm eV}\xspace}
\newcommand{\keV}{\ensuremath{\rm keV}\xspace}
\newcommand{\MeV}{\ensuremath{\rm MeV}\xspace}
\newcommand{\GeV}{\ensuremath{\rm GeV}\xspace}
\newcommand{\TeV}{\ensuremath{\rm TeV}\xspace}
\newcommand{\fm}{\ensuremath{\rm fm}\xspace}
\newcommand{\mm}{\ensuremath{\rm mm}\xspace}
\newcommand{\cm}{\ensuremath{\rm cm}\xspace}
\newcommand{\m}{\ensuremath{\rm m}\xspace}
\newcommand{\mum}{\ensuremath{\mu{\rm m}}\xspace}
\newcommand{\s}{\ensuremath{\rm s}\xspace}
\renewcommand{\d}{\ensuremath{\rm d}\xspace}
\newcommand{\ns}{\ensuremath{\rm ns}\xspace}
\newcommand{\ps}{\ensuremath{\rm ps}\xspace}
\newcommand{\mrad}{\ensuremath{\rm mrad}\xspace}
\newcommand{\mb}{\ensuremath{\rm mb}\xspace}
\newcommand{\ctau}{\ensuremath{{\rm c}\tau}\xspace}
\newcommand{\ctauapprox}[1]{\ctau $\approx$ #1 \mum}
\newcommand{\sqrts}{\ensuremath{\sqrt{s}}\xspace}
\newcommand{\compp}{{\ensuremath{\sqrt{s}} = 7 TeV}\xspace}
\newcommand{\compPb}{{\ensuremath{\sqrt{s}} = 8.16 TeV}\xspace}
\newcommand{\sqrtsNN}{\ensuremath{\sqrt{s_{\rm NN}}}\xspace}
\newcommand{\pt}{\ensuremath{{\it p}_{\rm T}}\xspace}
\newcommand{\come}[1]{{\ensuremath{\sqrt{s}} = #1 TeV}\xspace}
\newcommand{\comeNN}[1]{{\sqrtsNN = #1 TeV}\xspace}
\newcommand{\nch}{\ensuremath{N_{\rm ch}}\xspace}
\newcommand{\ntracklets}{\ensuremath{N_{\rm tracklets}}\xspace}
\newcommand{\ntrackletscorr}{\ensuremath{N^{\rm corr}_{\rm tracklets}}\xspace}
\newcommand{\dnchdeta}{\ensuremath{{\rm d}N_{\rm ch}/{\rm d}\eta}\xspace}
\newcommand{\dnchdpt}{\ensuremath{{\rm d}N_{\rm ch}/{\rm d}\pt}\xspace}
\newcommand{\dnchdy}{\ensuremath{{\rm d}N_{\rm ch}/{\rm d}y}\xspace}
\newcommand{\dntrackletsdeta}{\ensuremath{{\rm d}N_{\rm tracklets}/{\rm d}\eta}\xspace}
\newcommand{\avgntracklets}{\ensuremath{<N_{\rm tracklets}>}\xspace}
\newcommand{\avgntrackletscorr}{\ensuremath{<N^{\rm corr}_{\rm tracklets}>}\xspace}
\newcommand{\dnhfedeta}{\ensuremath{{\rm d}N_{\rm HFE}/{\rm d}\eta}\xspace}
\newcommand{\dndeta}{\ensuremath{{\rm d}N/{\rm d}\eta}\xspace}
\newcommand{\ptmore}[1]{{\pt $>$ #1 \GeVc}\xspace}
\newcommand{\ptless}[1]{{\pt $<$ #1 \GeVc}\xspace}
\newcommand{\ptrange}[2]{{#1 $<$ \pt $<$ #2 \GeVc}\xspace}
\newcommand{\etaless}[1]{\ensuremath{\left|\eta\right| < #1}\xspace}
\newcommand{\etarange}[2]{\ensuremath{#1 < \eta < #2}\xspace}
\newcommand{\yless}[1]{\ensuremath{\left|y\right| < #1}\xspace}
\newcommand{\yfid}{\ensuremath{y_{\rm fid}(\pt)}\xspace}
\newcommand{\yfidcut}{\ensuremath{\left|y\right| < y_{\rm fid}(\pt)}\xspace}
\newcommand{\dnchdetaless}[1]{\ensuremath{{\rm d}N_{\rm ch}/{\rm d}\eta|_{\etaless{#1}}}\xspace}
\newcommand{\zvertex}{\ensuremath{z_{\rm vtx}}\xspace}
\newcommand{\zvertexless}[1]{\ensuremath{\left|z_{\rm vtx}\right| < #1\ \cm}\xspace}
\newcommand{\zvertexout}[1]{\ensuremath{\left|z_{\rm vtx}\right| > #1\ \cm}\xspace}
\newcommand{\slfrac}[2]{\ensuremath{\left.#1\right/#2}\xspace}
\newcommand{\dedx}{\ensuremath{{\rm d}E/{\rm d}x}\xspace}
\newcommand{\asymmerr}[2]{\ensuremath{^{+#1}_{-#2}}\xspace}
\newcommand{\average}[1]{\ensuremath{\langle #1 \rangle}\xspace}
\newcommand{\nluminosity}[2]{\ensuremath{L_\text{int} = {#1}\pm{#2}\ \text{nb}^{-1}}\xspace}
\newcommand{\luminosity}{\ensuremath{L_\text{int}}\xspace}
\newcommand{\sphero}{\ensuremath{{S}_{\textit O}}\xspace}
\newcommand{\Dzero}{\ensuremath{{\rm D}^{0}}\xspace}
\newcommand{\Dzerobar}{\ensuremath{\overline{{\rm D}^{0}}}\xspace}
\newcommand{\DzeroNS}{\ensuremath{{\rm D}^{0}}} %NS = No space
\newcommand{\Dstarplus}{\ensuremath{{\rm D}^{*+}}\xspace}
\newcommand{\DstarplusNS}{\ensuremath{{\rm D}^{*+}}} %NS = No space
\newcommand{\Dplus}{\ensuremath{{\rm D}^{+}}\xspace}
\newcommand{\DplusNS}{\ensuremath{{\rm D}^{+}}} %NS = No space
\newcommand{\Piplus}{\ensuremath{{\pi}^{+}}\xspace}
\newcommand{\PiplusNS}{\ensuremath{{\pi}^{+}}} %NS = No space
\newcommand{\Piminus}{\ensuremath{{\pi}^{-}}\xspace}
\newcommand{\PiminusNS}{\ensuremath{{\pi}^{-}}}
\newcommand{\sPi}{\ensuremath{{\pi}}\xspace}
\newcommand{\Kplus}{\ensuremath{{\rm K}^{+}}\xspace}
\newcommand{\KplusNS}{\ensuremath{{\rm K}^{+}}}
\newcommand{\Kminus}{\ensuremath{{\rm K}^{-}}\xspace}
\newcommand{\KminusNS}{\ensuremath{{\rm K}^{-}}}
\newcommand{\sProton}{\ensuremath{\rm p}\xspace}
\newcommand{\pProtonNS}{\ensuremath{\rm p}}
\newcommand{\apProton}{\ensuremath{\overline{\rm p}}\xspace}
\newcommand{\apProtonNS}{\ensuremath{\overline{\rm p}}}
\newcommand{\sKzero}{\ensuremath{2{\rm K}^{0}_{S}}\xspace}
\newcommand{\pKzero}{\ensuremath{{\rm K}^{0}_{S}}\xspace}
\newcommand{\sXi}{\ensuremath{\Xi}\xspace}
\newcommand{\pXi}{\ensuremath{\Xi^{-}}\xspace}
\newcommand{\pXiNS}{\ensuremath{\Xi^{-}}}
\newcommand{\apXi}{\ensuremath{\overline{\Xi}^{+}}\xspace}
\newcommand{\apXiNS}{\ensuremath{\overline{\Xi}^{+}}}
\newcommand{\Jpsi}{\ensuremath{{\rm J}/\psi}\xspace}
\newcommand{\DtoKpi}{\ensuremath{{\Dzero}\to{\KminusNS}{\PiplusNS}}\xspace}
\newcommand{\DbartoKpi}{\ensuremath{{\Dzerobar}\to{\KplusNS}{\PiminusNS}}\xspace}
\newcommand{\DtoKpipi}{\ensuremath{{\Dplus}\to{\KminusNS}{\PiplusNS}{\PiplusNS}}\xspace}
\newcommand{\DstartoDpi}{\ensuremath{{\Dstarplus}\to{\DzeroNS}{\PiplusNS}}\xspace}
\newcommand{\brDtoKpi}{\ensuremath{{\rm 3.93} \pm {\rm 0.04}\%}\xspace}
\newcommand{\brDtoKpipi}{\ensuremath{{\rm 9.46} \pm {\rm 0.24}\%}\xspace}
\newcommand{\error}[1]{{\color{red}\bf \textsc{Wrong:} #1}}
\newcommand{\warning}[1]{{\color{red}\bf \textsc{Warning:} #1}}
\newcommand{\comments}[1]{{\color{blue}\bf \textsc{Comment:} #1}}
\newcommand{\correct}[2]{{\color{red}\sout{#1}}{\color{blue}\xspace#2}}
\newcommand{\cmnt}[1]{}
\newcommand{\fake}[1]{{\color{red}\bf#1}}
\newcommand{\alphas}{\ensuremath{\alpha_{\rm S}}\xspace}
\newcommand{\SPS}{\ensuremath{\rm Sp\bar{p}S}\xspace}
\newcommand{\Raa}{\ensuremath{R_{\rm AA}}\xspace}
\newcommand{\Rppb}{\ensuremath{R_{\rm pPb}}\xspace}
\newcommand{\Rpa}{\ensuremath{R_{\rm pPb}}\xspace}