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Perturbative predictions for the thrust ($\tau$) and heavy jet mass ($\rho$) distributions at LO, NLO and NNLO accuracy. The bands represent the renormalization scale uncertainty of our predictions corresponding to the range $\xi_R \in [0.5,2]$ around the central value of $\mu_0 = \sqrt{Q^2}$. The lower panels show the ratio of the (updated but unpublished -- see text) predictions of \cite{Weinzierl:2009ms} (SW) and \eerad~\cite{Ridder:2014wza} (GGGH) to \colorfulNNLO\ (this work). The bands on the lower panels show the relative scale uncertainty of our NNLO results.

Perturbative predictions for the thrust ($\tau$) and heavy jet mass ($\rho$) distributions at LO, NLO and NNLO accuracy. The bands represent the renormalization scale uncertainty of our predictions corresponding to the range $\xi_R \in [0.5,2]$ around the central value of $\mu_0 = \sqrt{Q^2}$. The lower panels show the ratio of the (updated but unpublished -- see text) predictions of \cite{Weinzierl:2009ms} (SW) and \eerad~\cite{Ridder:2014wza} (GGGH) to \colorfulNNLO\ (this work). The bands on the lower panels show the relative scale uncertainty of our NNLO results.

Same as \fig{fig:physical-omT+rho} for total ($B_T$) and wide ($B_W$) jet broadening.

Same as \fig{fig:physical-omT+rho} for total ($B_T$) and wide ($B_W$) jet broadening.

Same as \fig{fig:physical-omT+rho} for the $C$-parameter ($C_{\rm par}$) and the two-to-three jet transition parameter ($y_{23}$) in the Durham clustering algorithm.

Same as \fig{fig:physical-omT+rho} for the $C$-parameter ($C_{\rm par}$) and the two-to-three jet transition parameter ($y_{23}$) in the Durham clustering algorithm.

The $O\, C(O)$ coefficients of the thrust, heavy jet mass, total and wide jet broadening, $C$-parameter and two-to-three jet transition variable $y_{23}$ distributions. Lower panels show the ratio of the (updated but unpublished -- see text) predictions of \cite{Weinzierl:2009ms} (SW) and \eerad~\cite{Ridder:2014wza} (GGGH) to CoLoRFulNNLO (this work). The shaded bands on the lower panels represent the relative statistical uncertainties of our predictions due to Monte Carlo integrations.

The $O\, C(O)$ coefficients of the thrust, heavy jet mass, total and wide jet broadening, $C$-parameter and two-to-three jet transition variable $y_{23}$ distributions. Lower panels show the ratio of the (updated but unpublished -- see text) predictions of \cite{Weinzierl:2009ms} (SW) and \eerad~\cite{Ridder:2014wza} (GGGH) to CoLoRFulNNLO (this work). The shaded bands on the lower panels represent the relative statistical uncertainties of our predictions due to Monte Carlo integrations.

The $O\, C(O)$ coefficients of the thrust, heavy jet mass, total and wide jet broadening, $C$-parameter and two-to-three jet transition variable $y_{23}$ distributions. Lower panels show the ratio of the (updated but unpublished -- see text) predictions of \cite{Weinzierl:2009ms} (SW) and \eerad~\cite{Ridder:2014wza} (GGGH) to CoLoRFulNNLO (this work). The shaded bands on the lower panels represent the relative statistical uncertainties of our predictions due to Monte Carlo integrations.

The $O\, C(O)$ coefficients of the thrust, heavy jet mass, total and wide jet broadening, $C$-parameter and two-to-three jet transition variable $y_{23}$ distributions. Lower panels show the ratio of the (updated but unpublished -- see text) predictions of \cite{Weinzierl:2009ms} (SW) and \eerad~\cite{Ridder:2014wza} (GGGH) to CoLoRFulNNLO (this work). The shaded bands on the lower panels represent the relative statistical uncertainties of our predictions due to Monte Carlo integrations.

The $O\, C(O)$ coefficients of the thrust, heavy jet mass, total and wide jet broadening, $C$-parameter and two-to-three jet transition variable $y_{23}$ distributions. Lower panels show the ratio of the (updated but unpublished -- see text) predictions of \cite{Weinzierl:2009ms} (SW) and \eerad~\cite{Ridder:2014wza} (GGGH) to CoLoRFulNNLO (this work). The shaded bands on the lower panels represent the relative statistical uncertainties of our predictions due to Monte Carlo integrations.

The $O\, C(O)$ coefficients of the thrust, heavy jet mass, total and wide jet broadening, $C$-parameter and two-to-three jet transition variable $y_{23}$ distributions. Lower panels show the ratio of the (updated but unpublished -- see text) predictions of \cite{Weinzierl:2009ms} (SW) and \eerad~\cite{Ridder:2014wza} (GGGH) to CoLoRFulNNLO (this work). The shaded bands on the lower panels represent the relative statistical uncertainties of our predictions due to Monte Carlo integrations.

The distribution of jet cone energy fraction (JCEF) at LO, NLO and NNLO accuracy in perturbative QCD. The bands represent the variation of the renormalization scale in the range $\xi_R = \mu/\mu_0 \in [0.5,2]$ around the central value of $\mu_0=\sqrt{Q^2}$. The lower panel shows the relative scale dependence at NNLO accuracy.

The distribution of the NNLO coefficient for jet cone energy fraction (JCEF). The error bars represent the statistical uncertainty of the Monte Carlo integrations.