$v_{2,2}^{unsub}$ and $v_{2,2}$ as a function of $\Delta\eta$ calculated from the 2-D per-trigger yields in figure 4(a) and 4(b), respectively.

$v_{3,3}^{unsub}$ and $v_{3,3}$ as a function of $\Delta\eta$ calculated from the 2-D per-trigger yields in figure 4(a) and 4(b), respectively.

$v_{4,4}^{unsub}$ and $v_{4,4}$ as a function of $\Delta\eta$ calculated from the 2-D per-trigger yields in figure 4(a) and 4(b), respectively.

The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.

The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.

The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.

The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.

The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.

The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.

The per-trigger yield distributions $Y^{corr}(\Delta\phi)$ and $Y^{recoil}(\Delta\phi)$ for events with $N_{ch}^{rec} \geq$ 220 in the long-range region $|\Delta\eta| >$ 2.

Integrated per-trigger yield, $Y_{int}$, on the near-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the near-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the near-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the near-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the near-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the away-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the away-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the away-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the away-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

Integrated per-trigger yield, $Y_{int}$, on the away-side as a function of $p_{T}^{a}$ for 1 $< p_{T}^{b} <$ 3 GeV.

The integrated per-trigger yield, Y_{int}, on the near-side, the away-side and their difference and Y_{int} from the recoil as a function of event activity. Errors are statistical.

The integrated per-trigger yield, Y_{int}, on the near-side, the away-side and their difference and Y_{int} from the recoil as a function of event activity. Errors are statistical.

The Fourier coefficients $v_{n}$ as a function of $p_{T}^{a}$ extracted from the correlation functions, before and after the subtraction of the recoil component.

The Fourier coefficients $v_{n}$ as a function of $p_{T}^{a}$ extracted from the correlation functions, before and after the subtraction of the recoil component.

The Fourier coefficients $v_{n}$ as a function of $p_{T}^{a}$ extracted from the correlation functions, before and after the subtraction of the recoil component.

$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.

$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.

$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.

$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.

$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.

$v_{2}$, $v_{3}$, $v_{4}$ and $v_{5}$ as a function of $p_T^a$ for 1 $< p_{T}^{b} <$ 3 GeV for different $N_{ch}^{rec}$ intervals.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{2}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The values of factorization variable $r_{3}$ defined by Eq.(11) before and after the subtraction of the recoil component. Errors are total experimental uncertainties.

The centrality dependence of $v_{2}$ as a function of $N_{ch}^{rec}$. Values from before and after the recoil subtraction are included.

The centrality dependence of $v_{3}$ as a function of $N_{ch}^{rec}$. Values from before and after the recoil subtraction are included.

The centrality dependence of $v_{4}$ as a function of $N_{ch}^{rec}$. Values from before and after the recoil subtraction are included.

The centrality dependence of $v_{2}$ as a function of $E_{T}^{Pb}$. Values from before and after the recoil subtraction are included.

The centrality dependence of $v_{3}$ as a function of $E_{T}^{Pb}$. Values from before and after the recoil subtraction are included.

The centrality dependence of $v_{4}$ as a function of $E_{T}^{Pb}$. Values from before and after the recoil subtraction are included.

The $v_{2}$ as a function of $E_{T}^{Pb}$ obtained indirectly by mapping from the $N_{ch}^{rec}-dependence of $v_{2}$ using the correlation data shown in Fig. 2(b).

The $v_{3}$ as a function of $E_{T}^{Pb}$ obtained indirectly by mapping from the $N_{ch}^{rec}-dependence of $v_{3}$ using the correlation data shown in Fig. 2(b).

The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC before recoil subtraction, $v_{1,1}^{unsub}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic of 2PC after recoil subtraction, $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic $v_1$ obtained using factorization from $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic $v_1$ obtained using factorization from $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

The first-order harmonic $v_1$ obtained using factorization from $v_{1,1}$, as a function of $p_T^a$ for different $p_T^b$ ranges for events with $N_{ch}^{rec} \geq$ 220.

$v_{2}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method.

$v_{2}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method, after the scaling.

$v_{3}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method.

$v_{3}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method, after the scaling.

$v_{4}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method.

$v_{4}$ for Pb+Pb collisions in 55-60% centrality interval obtained using an EP method, after the scaling.

Correlation between $E_{T}^{FCal}$ and $N_{ch}^{rec}$ for MB events (without weighting) and MB+HMT events (with weighting), errors are statistical.

Production rate for PI0 production in the rapidity range -9.4 to -9.6.

Production rate for PI0 production in the rapidity range -9.6 to -10.0.

Production rate for PI0 production in the rapidity range -10.0 to -11.0.

Single differential production cross sections of prompt J/PSI mesons and of J/PSI from B decay as a function of rapidity in the BACKWARD region. The errors shown are statistical and the uncorrelated and correlated components of the systematic uncertainties.

Double differential production cross sections of prompt J/PSI mesons as a function of transverse momentum and rapidity in the FORWARD region. The errors shown are statistical and the uncorrelated and correlated components of the systematic uncertainties.

Double differential production cross sections of J/PSI mesons from B decays as a function of transverse momentum and rapidity in the FORWARD region. The errors shown are statistical and the uncorrelated and correlated components of the systematic uncertainties.

The nuclear modification factor RpPB for PT < 14 GeV/c in the BACKWARD and FORWARD regions.

The FORWARD/BACKWARD production ratio R(FB) as a function of rapidity for PT < 14 GeV/c.

The FORWARD/BACKWARD production ratioo (R(FB) as a function of PT with |yrap|=2.5-4.0.

The measured inclusive jet double-differential cross section in the rapidity bin 1.2 <= |y| < 2.1 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 2.1 <= |y| < 2.8 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 2.8 <= |y| < 3.6 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 3.6 <= |y| < 4.4 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin |y| < 0.3 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 0.3 <= |y| < 0.8 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 0.8 <= |y| < 1.2 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 1.2 <= |y| < 2.1 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 2.1 <= |y| < 2.8 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 2.8 <= |y| < 3.6 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 3.6 <= |y| < 4.4 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin |y| < 0.3 for anti-kt jets with R = 0.4 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 0.3 <= |y| < 0.8 for anti-kt jets with R = 0.4 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 0.8 <= |y| < 1.2 for anti-kt jets with R = 0.4 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 1.2 <= |y| < 2.1 for anti-kt jets with R = 0.4 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 2.1 <= |y| < 2.8 for anti-kt jets with R = 0.4 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 2.8 <= |y| < 3.6 for anti-kt jets with R = 0.4 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 3.6 <= |y| < 4.4 for anti-kt jets with R = 0.4 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin |y| < 0.3 for anti-kt jets with R = 0.6 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 0.3 <= |y| < 0.8 for anti-kt jets with R = 0.6 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 0.8 <= |y| < 1.2 for anti-kt jets with R = 0.6 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 1.2 <= |y| < 2.1 for anti-kt jets with R = 0.6 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 2.1 <= |y| < 2.8 for anti-kt jets with R = 0.6 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 2.8 <= |y| < 3.6 for anti-kt jets with R = 0.6 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 3.6 <= |y| < 4.4 for anti-kt jets with R = 0.6 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin |y| < 0.3 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 0.3 <= |y| < 0.8 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 0.8 <= |y| < 1.2 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 1.2 <= |y| < 2.1 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 2.1 <= |y| < 2.8 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 2.8 <= |y| < 3.6 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 3.6 <= |y| < 4.4 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin |y| < 0.3 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 0.3 <= |y| < 0.8 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 0.8 <= |y| < 1.2 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 1.2 <= |y| < 2.1 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 2.1 <= |y| < 2.8 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 2.8 <= |y| < 3.6 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 3.6 <= |y| < 4.4 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The second flow harmonic measured with the two-particle cumulants as a function of transverse momentum in the event activity bin of >80 GeV.

The second flow harmonic measured with the four-particle cumulants as a function of transverse momentum in the event activity bin of 25-40 GeV.

The second flow harmonic measured with the four-particle cumulants as a function of transverse momentum in the event activity bin of 40-55 GeV.

The second flow harmonic measured with the four-particle cumulants as a function of transverse momentum in the event activity bin of 55-80 GeV.

The second flow harmonic measured with the four-particle cumulants as a function of transverse momentum in the event activity bin of >80 GeV.

The second-order harmonic, v2, integrated over pT and eta, calculated with two-particle cumulants as a function of Sum ET^Pb.

The second-order harmonic, v2, integrated over pT and eta, calculated with four-particle cumulants as a function of Sum ET^Pb.

Distribution of per-trigger yield, Y(DELTA(PHI)), in the peripheral and the central event activity classes and their differences, for 2 < pT(a) < 3 GeV and 0.5 < pT(b) < 4 GeV.

Distribution of per-trigger yield, Y(DELTA(PHI)), in the peripheral and the central event activity classes and their differences, for 3 < pT(a) < 4 GeV and 0.5 < pT(b) < 4 GeV.

Distribution of per-trigger yield, Y(DELTA(PHI)), in the peripheral and the central event activity classes and their differences, for 4 < pT(a) < 5 GeV and 0.5 < pT(b) < 4 GeV.

Integrated per-trigger yields, Yint, versus pT(a) for 0.5 < pT(b) < 4 GeV, in the SUM(ET(PB)) > 80 GeV event class, on the near-side, |Delta(phi)| < PI/3.

Integrated per-trigger yields, Yint, versus pT(a) for 0.5 < pT(b) < 4 GeV, in the SUM(ET(PB)) = 55-80 GeV event class, on the near-side, |Delta(phi)| < PI/3.

Integrated per-trigger yields, Yint, versus pT(a) for 0.5 < pT(b) < 4 GeV, in the SUM(ET(PB)) = 25-55 GeV event class, on the near-side, |Delta(phi)| < PI/3.

Integrated per-trigger yields, Yint, versus pT(a) for 0.5 < pT(b) < 4 GeV, in the SUM(ET(PB)) < 20 GeV event class, on the near-side, |Delta(phi)| < PI/3.

Difference of the yield in the SUM(ET(PB)) > 80 GeV event class from that in the SUM(ET(PB)) < 20 GeV event class, on the near-side, |Delta(phi)| < PI/3.

Difference of the yield in the SUM(ET(PB)) = 55-80 GeV event class from that in the SUM(ET(PB)) < 20 GeV event class, on the near-side, |Delta(phi)| < PI/3.

Difference of the yield in the SUM(ET(PB)) = 25-55 GeV event class from that in the SUM(ET(PB)) < 20 GeV event class, on the near-side, |Delta(phi)| < PI/3.

Integrated per-trigger yields, Yint, versus pT(a) for 0.5 < pT(b) < 4 GeV, in the SUM(ET(PB)) > 80 GeV event class, on the away-side, |Delta(phi)| > 2*PI/3.

Integrated per-trigger yields, Yint, versus pT(a) for 0.5 < pT(b) < 4 GeV, in the SUM(ET(PB)) = 55-80 GeV event class, on the away-side, |Delta(phi)| > 2*PI/3.

Integrated per-trigger yields, Yint, versus pT(a) for 0.5 < pT(b) < 4 GeV, in the SUM(ET(PB)) = 25-55 GeV event class, on the away-side, |Delta(phi)| > 2*PI/3.

Integrated per-trigger yields, Yint, versus pT(a) for 0.5 < pT(b) < 4 GeV, in the SUM(ET(PB)) < 20 GeV event class, on the away-side, |Delta(phi)| > 2*PI/3.

Difference of the yield in the SUM(ET(PB)) > 80 GeV event class from that in the SUM(ET(PB)) < 20 GeV event class, on the away-side, |Delta(phi)| > 2*PI/3.

Difference of the yield in the SUM(ET(PB)) = 55-80 GeV event class from that in the SUM(ET(PB)) < 20 GeV event class, on the away-side, |Delta(phi)| > 2*PI/3.

Difference of the yield in the SUM(ET(PB)) = 25-55 GeV event class from that in the SUM(ET(PB)) < 20 GeV event class, on the away-side, |Delta(phi)| > 2*PI/3.

The pT(a) dependence of c2 for 0.5 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of c2 for 0.5 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of c2 for 0.5 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s2 for 0.5 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s2 for 0.5 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s2 for 0.5 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of c3 for 0.5 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of c3 for 0.5 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of c3 for 0.5 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s3 for 0.5 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s3 for 0.5 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s3 for 0.5 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of c2 for 1 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of c2 for 1 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of c2 for 1 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s2 for 1 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s2 for 1 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s2 for 1 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of c3 for 1 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of c3 for 1 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of c3 for 1 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s3 for 1 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s3 for 1 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s3 for 1 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of c2 for 1.5 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of c2 for 1.5 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of c2 for 1.5 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s2 for 1.5 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s2 for 1.5 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s2 for 1.5 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of c3 for 1.5 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of c3 for 1.5 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of c3 for 1.5 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s3 for 1.5 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s3 for 1.5 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s3 for 1.5 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of c2 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of c2 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of c2 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s2 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s2 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s2 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of c3 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of c3 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of c3 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s3 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s3 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s3 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of c2 for 1 < pT(b) < 2, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of c2 for 1 < pT(b) < 2, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of c2 for 1 < pT(b) < 2, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s2 for 1 < pT(b) < 2, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s2 for 1 < pT(b) < 2, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s2 for 1 < pT(b) < 2, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of c3 for 1 < pT(b) < 2, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of c3 for 1 < pT(b) < 2, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of c3 for 1 < pT(b) < 2, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s3 for 1 < pT(b) < 2, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s3 for 1 < pT(b) < 2, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s3 for 1 < pT(b) < 2, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of c2 for 2 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of c2 for 2 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of c2 for 2 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s2 for 2 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s2 for 2 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s2 for 2 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of c3 for 2 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of c3 for 2 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of c3 for 2 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s3 for 2 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s3 for 2 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s3 for 2 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

Integrated per-trigger yield, Yint, for 0.5 < pT(a,b) < 4 GeV, measured in intervals of SUM(ET(PB)), for the near-side (|Delta(phi)| < PI/3), away-side (|Delta(phi)| > 2*PI/3) and the difference between them, DELTA(Yint).

Integrated per-trigger yield, Yint, for 1 < pT(a,b) < 4 GeV, measured in intervals of SUM(ET(PB)), for the near-side (|Delta(phi)| < PI/3), away-side (|Delta(phi)| > 2*PI/3) and the difference between them, DELTA(Yint).

Integrated per-trigger yield, Yint, for 0.5 < pT(a,b) < 4 GeV, measured in intervals of Nch, where Nch represents the charged-particle multiplicity measured over |eta| < 2.5 with pT > 0.4 GeV, for the near-side (|Delta(phi)| < PI/3), away-side (|Delta(phi)| > 2*PI/3) and the difference between them, DELTA(Yint).

Integrated per-trigger yield, Yint, for 1 < pT(a,b) < 4 GeV, measured in intervals of Nch, where Nch represents the charged-particle multiplicity measured over |eta| < 2.5 with pT > 0.4 GeV, for the near-side (|Delta(phi)| < PI/3), away-side (|Delta(phi)| > 2*PI/3) and the difference between them, DELTA(Yint).

The pT(a) dependence of s2 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s2 for 1 < pT(b) < 2, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s2 for 2 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s2 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s2 for 1 < pT(b) < 2, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s2 for 2 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s2 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s2 for 1 < pT(b) < 2, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s2 for 2 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s3 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s3 for 1 < pT(b) < 2, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s3 for 2 < pT(b) < 4, in the SUM(ET(PB)) > 80 GeV event class.

The pT(a) dependence of s3 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s3 for 1 < pT(b) < 2, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s3 for 2 < pT(b) < 4, in the SUM(ET(PB)) = 55-80 GeV event class.

The pT(a) dependence of s3 for 0.5 < pT(b) < 1, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s3 for 1 < pT(b) < 2, in the SUM(ET(PB)) = 25-55 GeV event class.

The pT(a) dependence of s3 for 2 < pT(b) < 4, in the SUM(ET(PB)) = 25-55 GeV event class.

Distribution of per-trigger yield, Y(DELTA(PHI)), in the peripheral and the central event activity classes and their differences, for 3 < pT(a) < 4 GeV and 0.3 < pT(b) < 0.5 GeV.

Distribution of per-trigger yield, Y(DELTA(PHI)), in the peripheral and the central event activity classes and their differences, for 3 < pT(a) < 4 GeV and 0.5 < pT(b) < 1 GeV.

Distribution of per-trigger yield, Y(DELTA(PHI)), in the peripheral and the central event activity classes and their differences, for 3 < pT(a) < 4 GeV and 1 < pT(b) < 2 GeV.

Distribution of per-trigger yield, Y(DELTA(PHI)), in the peripheral and the central event activity classes and their differences, for 3 < pT(a) < 4 GeV and 2 < pT(b) < 3 GeV.

Distribution of per-trigger yield, Y(DELTA(PHI)), in the peripheral and the central event activity classes and their differences, for 2 < pT(a) < 3 GeV and 0.3 < pT(b) < 0.5 GeV.

Distribution of per-trigger yield, Y(DELTA(PHI)), in the peripheral and the central event activity classes and their differences, for 2 < pT(a) < 3 GeV and 0.5 < pT(b) < 1 GeV.

Distribution of per-trigger yield, Y(DELTA(PHI)), in the peripheral and the central event activity classes and their differences, for 2 < pT(a) < 3 GeV and 1 < pT(b) < 2 GeV.

Distribution of per-trigger yield, Y(DELTA(PHI)), in the peripheral and the central event activity classes and their differences, for 2 < pT(a) < 3 GeV and 2 < pT(b) < 3 GeV.

Distribution of per-trigger yield, Y(DELTA(PHI)), in the peripheral and the central event activity classes and their differences, for 1 < pT(a) < 2 GeV and 0.3 < pT(b) < 0.5 GeV.

Distribution of per-trigger yield, Y(DELTA(PHI)), in the peripheral and the central event activity classes and their differences, for 1 < pT(a) < 2 GeV and 0.5 < pT(b) < 1 GeV.

Distribution of per-trigger yield, Y(DELTA(PHI)), in the peripheral and the central event activity classes and their differences, for 1 < pT(a) < 2 GeV and 1 < pT(b) < 2 GeV.

Distribution of per-trigger yield, Y(DELTA(PHI)), in the peripheral and the central event activity classes and their differences, for 0.5 < pT(a) < 1 GeV and 0.3 < pT(b) < 0.5 GeV.

Distribution of per-trigger yield, Y(DELTA(PHI)), in the peripheral and the central event activity classes and their differences, for 0.5 < pT(a) < 1 GeV and 0.5 < pT(b) < 1 GeV.

Total production cross sections of D mesons, extrapolated to the full phase space. The second (sys) error is the from the luminosity uncertainty, the third from the branching-ratio uncertainties and the fourth is from the extrapolation uncertainty.

The ratio, Pv, of cdbar D mesons produced in a vector state to those produced in a vector or a pseudoscalar state. The second (sys) error is the the branching-ratio uncertainties and the third is from the extrapolation uncertainty.

The weighted average of the total charm production cross section. The second (sys) error is the from the branching-ratio uncertainties, the third is from the Fragmentation Function uncertainties, the fourth is from the luminosity uncertainty and the fifth is from the extrapolation uncertainty.

Corrected two particle RCORR distribution as a function of Delta(PHI) obtained by integrating the foreground and background distributions over Delta(ETARAP) between 0 and 2.

Corrected two particle RCORR distribution as a function of Delta(PHI) obtained by integrating the foreground and background distributions over Delta(ETARAP) between 2 and 5.

Number density as a function of the leading charged-particle PT at a centre-mass-energy of 7000 GeV for events having charged-particle PT > 0.5 GeV. The data is shown for the three azimuthal regions.

Number density as a function of the leading charged-particle PT at a centre-mass-energy of 900 GeV for events having charged-particle PT > 1.0 GeV. The data is shown for the three azimuthal regions.

Number density as a function of the leading charged-particle PT at a centre-mass-energy of 7000 GeV for events having charged-particle PT > 1.0 GeV. The data is shown for the three azimuthal regions.

The summed PT as a function of the leading charged-particle PT at a centre-mass-energy of 900 GeV for events having charged-particle PT > 0.15 GeV. The data is shown for the three azimuthal regions.

The summed PT as a function of the leading charged-particle PT at a centre-mass-energy of 7000 GeV for events having charged-particle PT > 0.15 GeV. The data is shown for the three azimuthal regions.

The summed PT as a function of the leading charged-particle PT at a centre-mass-energy of 900 GeV for events having charged-particle PT > 0.5 GeV. The data is shown for the three azimuthal regions.

The summed PT as a function of the leading charged-particle PT at a centre-mass-energy of 7000 GeV for events having charged-particle PT > 0.5 GeV. The data is shown for the three azimuthal regions.

The summed PT as a function of the leading charged-particle PT at a centre-mass-energy of 900 GeV for events having charged-particle PT > 1.0 GeV. The data is shown for the three azimuthal regions.

The summed PT as a function of the leading charged-particle PT at a centre-mass-energy of 7000 GeV for events having charged-particle PT > 1.0 GeV. The data is shown for the three azimuthal regions.

The azimuthal correlation as a function of DPHI, the azimuthal different between tracks and the leading PT track, for events having PT > 0.15 GeV and the leading track PT in the range 0.5-1.5. The data is shown for centre-of-mass energies of 0.9 and 7 TeV.

The azimuthal correlation as a function of DPHI, the azimuthal different between tracks and the leading PT track, for events having PT > 0.15 GeV and the leading track PT in the range 2.0-4.0. The data is shown for centre-of-mass energies of 0.9 and 7 TeV.

The azimuthal correlation as a function of DPHI, the azimuthal different between tracks and the leading PT track, for events having PT > 0.15 GeV and the leading track PT in the range 4.0-6.0. The data is shown for centre-of-mass energies of 0.9 and 7 TeV.

The azimuthal correlation as a function of DPHI, the azimuthal different between tracks and the leading PT track, for events having PT > 0.15 GeV and the leading track PT in the range 6.0-10.0. The data is shown for centre-of-mass energies of 0.9 and 7 TeV.

The azimuthal correlation as a function of DPHI, the azimuthal different between tracks and the leading PT track, for events having PT > 0.5 GeV and the leading track PT in the range 0.5-1.5. The data is shown for centre-of-mass energies of 0.9 and 7 TeV.

The azimuthal correlation as a function of DPHI, the azimuthal different between tracks and the leading PT track, for events having PT > 0.5 GeV and the leading track PT in the range 2.0-4.0. The data is shown for centre-of-mass energies of 0.9 and 7 TeV.

The azimuthal correlation as a function of DPHI, the azimuthal different between tracks and the leading PT track, for events having PT > 0.5 GeV and the leading track PT in the range 4.0-6.0. The data is shown for centre-of-mass energies of 0.9 and 7 TeV.

The azimuthal correlation as a function of DPHI, the azimuthal different between tracks and the leading PT track, for events having PT > 0.5 GeV and the leading track PT in the range 6.0-10.0. The data is shown for centre-of-mass energies of 0.9 and 7 TeV.

The azimuthal correlation as a function of DPHI, the azimuthal different between tracks and the leading PT track, for events having PT > 1.0 GeV and the leading track PT in the range 2.0-4.0. The data is shown for centre-of-mass energies of 0.9 and 7 TeV.

The azimuthal correlation as a function of DPHI, the azimuthal different between tracks and the leading PT track, for events having PT > 1.0 GeV and the leading track PT in the range 4.0-6.0. The data is shown for centre-of-mass energies of 0.9 and 7 TeV.

The azimuthal correlation as a function of DPHI, the azimuthal different between tracks and the leading PT track, for events having PT > 1.0 GeV and the leading track PT in the range 6.0-10.0. The data is shown for centre-of-mass energies of 0.9 and 7 TeV.