Missing ET distribution in SR2B for stop GMSB model (data+/-stat, bkg+/-(stat+syst), signal+/-stat), m(stop1)=500 GeV, m(neutralino1)=400 GeV.

Missing ET distribution in SR2C for stop GMSB model (data+/-stat, bkg+/-(stat+syst), signal+/-stat), m(stop1)=500 GeV, m(neutralino1)=400 GeV.

met_sr3a (data+/-stat, bkg+/-(stat+syst), signal+/-stat).

met_sr3b (data+/-stat, bkg+/-(stat+syst), signal+/-stat).

Expected exclusion limits at 95% CL for stop2 grid.

Expected exclusion limits +1sigma at 95% CL for stop2 grid.

Expected exclusion limits -1sigma at 95% CL for stop2 grid.

Observed exclusion limits at 95% CL for stop2 grid.

Observed exclusion limits +1sigma SUSY cross section uncertainty at 95% CL for stop2 grid.

Observed exclusion limits -1sigma SUSY cross section uncertainty at 95% CL for stop2 grid.

t2_350_n1_20_Observed.

t2_350_n1_20_Expected.

t2_500_n1_20_Observed.

t2_500_n1_20_Expected.

t2_500_n1_120_Observed.

t2_500_n1_120_Expected.

Expected exclusion limits at 95% CL for stop GMSB model.

Expected exclusion limits +1sigma at 95% CL for stop GMSB model.

Expected exclusion limits -1sigma at 95% CL for stop GMSB model.

Observed exclusion limits at 95% CL for stop GMSB model.

Observed exclusion limits +1sigma SUSY cross section uncertainty at 95% CL for stop GMSB model.

Observed exclusion limits -1sigma SUSY cross section uncertainty at 95% CL for stop GMSB model.

met_3l2j (data+/-stat, bkg+/-(stat+syst), signal+/-stat).

met_3l3j (data+/-stat, bkg+/-(stat+syst), signal+/-stat).

The best expected signal region for stop2 model, where 1 and 2 mean SR3A and SR3B.

The best expected signal region for stop GMSB model, where 1 and 2 mean SR2A and SR2B.

The best expected signal region for stop2 mass 350 GeV and neutralino1 mass 20 GeV, where 1 and 2 mean SR3A and SR3B.

The best expected signal region for stop2 mass 500 GeV and neutralino1 mass 20 GeV, where 1 and 2 mean SR3A and SR3B.

The best expected signal region for stop2 mass 500 GeV and neutralino1 mass 120 GeV, where 1 and 2 mean SR3A and SR3B.

Observed upper limit on the signal cross section for stop2 grid.

Number of generated MC events for stop Natural GMSB model.

Cross section for stop Natural GMSB model.

xsec_stop2.

Ntot_stop2.

Acceptance of stop GMSB model for SR2A.

Efficiency of stop GMSB model for SR2A.

Number of expected signal events of stop GMSB model for SR2A.

Total systematic uncertainty of stop GMSB model for SR2A.

Observed CL_s of stop GMSB model for SR2A.

Expected CL_s of stop GMSB model for SR2A.

Acceptance of stop GMSB model for SR2B.

Efficiency of stop GMSB model for SR2B.

Number of expected signal events of stop GMSB model for SR2B.

Total systematic uncertainty of stop GMSB model for SR2B.

Observed CL_s of stop GMSB model for SR2B.

Expected CL_s of stop GMSB model for SR2B.

Acceptance of stop GMSB model for SR2C.

Efficiency of stop GMSB model for SR2C.

Number of expected signal events of stop GMSB model for SR2C.

Total systematic uncertainty of stop GMSB model for SR2C.

Observed CL_s of stop GMSB model for SR2C.

Expected CL_s of stop GMSB model for SR2C.

Nexp_SR3A.

RelUnc_SR3A.

Acc_SR3A.

Eff_SR3A.

CLsExp_SR3A.

CLs_SR3A.

Nexp_SR3B.

RelUnc_SR3B.

Acc_SR3B.

Eff_SR3B.

CLsExp_SR3B.

CLs_SR3B.

Sample fit projections onto the $q_{out}$, $q_{side}$, and $q_{long}$ axes respectively for four angular bins relative to the reaction. These projections are from results for 10-20% central, 19.6 GeV Au+Au collisions with 0.15 < $k_T$ < 0.6 GeV/c.

Energy dependence of the HBT parameters for central Au+Au, Pb+Pb, and Pb+Au collisions at mid-rapidity and $\langle k_T \rangle \approx 0.22$ GeV/c. Errors on NA44, NA49, WA98, and CERES, points include systematic errors.The systematic errors for STAR points at all energies (from Table II) are of similar size to error bar for 39 GeV, shown as a representative example. Errors on other results are statistical only, to emphasize the trend.

The $\langle m_T \rangle$ dependence of $R_{out}$, $R_{side}$ and $R_{long}$ for all energies at 0-5% centrality. Errors are statistical only. These plot shows the difference (between $R_{out}$ and $R_{side}$) and the ratio $R_{out}$ / $R_{side}$ respectively.

The $\langle m_T \rangle$ dependence of $R_{out}$, $R_{side}$ and $R_{long}$ for each energy and multiple centralities. Errors are statistical only.

The dependence of the HBT radii on multiplicity,$\langle dN_{ch}/d\eta \rangle^{1/3}$, for $k_T\approx 0.22$ GeV/c and$k_T\approx 0.39$ GeV/c. Results are for Au+Au collisions at STAR at 7 GeV. Errors are statistical only.

The dependence of the HBT radii on multiplicity,$\langle dN_{ch}/d\eta \rangle^{1/3}$, for $k_T\approx 0.22$ GeV/c and$k_T\approx 0.39$ GeV/c. Results are for Au+Au collisions at STAR at 11.5 GeV. Errors are statistical only.

The dependence of the HBT radii on multiplicity,$\langle dN_{ch}/d\eta \rangle^{1/3}$, for $k_T\approx 0.22$ GeV/c and$k_T\approx 0.39$ GeV/c. Results are for Au+Au collisions at STAR at 19.6 GeV. Errors are statistical only.

The dependence of the HBT radii on multiplicity,$\langle dN_{ch}/d\eta \rangle^{1/3}$, for $k_T\approx 0.22$ GeV/c and$k_T\approx 0.39$ GeV/c. Results are for Au+Au collisions at STAR at 27 GeV. Errors are statistical only.

The dependence of the HBT radii on multiplicity,$\langle dN_{ch}/d\eta \rangle^{1/3}$, for $k_T\approx 0.22$ GeV/c and$k_T\approx 0.39$ GeV/c. Results are for Au+Au collisions at STAR at 39 GeV. Errors are statistical only.

The dependence of the HBT radii on multiplicity,$\langle dN_{ch}/d\eta \rangle^{1/3}$, for $k_T\approx 0.22$ GeV/c and$k_T\approx 0.39$ GeV/c. Results are for Au+Au collisions at STAR at 62.4 GeV. Errors are statistical only.

The dependence of the HBT radii on multiplicity,$\langle dN_{ch}/d\eta \rangle^{1/3}$, for $k_T\approx 0.22$ GeV/c and$k_T\approx 0.39$ GeV/c. Results are for Au+Au collisions at STAR at 200 GeV. Errors are statistical only.

The dependence of the HBT radii on multiplicity,$\langle dN_{ch}/d\eta \rangle^{1/3}$, for $k_T\approx 0.22$ GeV/c and$k_T\approx 0.39$ GeV/c. Results are for Si+Al collisions at E802, Pb+Au at CERES, Pb+Pb at ALICE. Errors are statistical only.

The beam energy dependence of the volume of the regions of homogeneity at kinetic freeze-out in central Au+Au, Pb+Pb and Pb+Au collisions with $k_T\approx 0.22$ GeV/c.

The lifetime, $\tau$, of the system as a function of beam energy for central Au+Au collisions assuming a temperature of T = 0.12 GeV at kinetic freeze-out.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at mid-rapidity (−0.5 < y < 0.5), in 7.7 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c for the azimuthally integrated radii and the 0th-order Fourier coefficients. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at mid-rapidity (−0.5 < y < 0.5), in 7.7 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c, from the HHLW method (Gaussian fits to each angular bin) and a single global fit to all angular bins to directly. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at backward(−1<y<−0.5), forward(0.5<y<1)and mid(−0.5<y< 0.5) rapidity, in 7.7 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c using the global fit method. Error bars include only statistical uncertain- ties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at mid-rapidity (−0.5 < y < 0.5), in 11.5 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c for the azimuthally integrated radii and the 0th-order Fourier coefficients. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at mid-rapidity (−0.5 < y < 0.5), in 11.5 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c, from the HHLW method (Gaussian fits to each angular bin) and a single global fit to all angular bins to directly. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at backward(−1<y<−0.5), forward(0.5<y<1) and mid(−0.5<y< 0.5) rapidity, in 11.5 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c using the global fit method. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at mid-rapidity (−0.5 < y < 0.5), in 19.6 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c for the azimuthally integrated radii and the 0th-order Fourier coefficients. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at mid-rapidity (−0.5 < y < 0.5), in 19.6 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c, from the HHLW method (Gaussian fits to each angular bin) and a single global fit to all angular bins to directly. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at backward(−1<y<−0.5), forward(0.5<y<1) and mid(−0.5<y< 0.5) rapidity, in 19.6 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c using the global fit method. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at mid-rapidity (−0.5 < y < 0.5), in 27 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c for the azimuthally integrated radii and the 0th-order Fourier coefficients. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at mid-rapidity (−0.5 < y < 0.5), in 27 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c, from the HHLW method (Gaussian fits to each angular bin) and a single global fit to all angular bins to directly. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at backward(−1<y<−0.5), forward(0.5<y<1) and mid(−0.5<y< 0.5) rapidity, in 27 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c using the global fit method. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at mid-rapidity (−0.5 < y < 0.5), in 39 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c for the azimuthally integrated radii and the 0th-order Fourier coefficients. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at mid-rapidity (−0.5 < y < 0.5), in 39 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c, from the HHLW method (Gaussian fits to each angular bin) and a single global fit to all angular bins to directly. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at backward(−1<y<−0.5), forward(0.5<y<1) and mid(−0.5<y< 0.5) rapidity, in 39 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c using the global fit method. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at mid-rapidity (−0.5 < y < 0.5), in 62.4 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c for the azimuthally integrated radii and the 0th-order Fourier coefficients. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at mid-rapidity (−0.5 < y < 0.5), in 62.4 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c, from the HHLW method (Gaussian fits to each angular bin) and a single global fit to all angular bins to directly. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at backward(−1<y<−0.5), forward(0.5<y<1) and mid(−0.5<y< 0.5) rapidity, in 62.4 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c using the global fit method. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at mid-rapidity (−0.5 < y < 0.5), in 200 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c for the azimuthally integrated radii and the 0th-order Fourier coefficients. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at mid-rapidity (−0.5 < y < 0.5), in 200 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c, from the HHLW method (Gaussian fits to each angular bin) and a single global fit to all angular bins to directly. Error bars include only statistical uncertainties.

Centrality dependence of the Fourier coefficients that describe azimuthal oscillations of the HBT radii, at backward(−1<y<−0.5), forward(0.5<y<1) and mid(−0.5<y< 0.5) rapidity, in 200 GeV collisions with ⟨$k_T$⟩ ≈ 0.31 GeV/c using the global fit method. Error bars include only statistical uncertainties.

Beam energy dependence of the $R_{ol,0}^2$ cross term for forward and backward rapidity with ⟨$k_T$⟩ ≈ 0.31 GeV/c.

The eccentricity of the collisions at kinetic freez-out, εF , as a function of initial eccentricity relative to the participant plane, ε$_{PP}$, at mid-rapidity. All results are for ⟨$k_T$⟩ ≈ 0.31 GeV/c. Error bars include only statistical uncertainties. The line has a slope of one indicating no change in shape.

The dependence of the kinetic freeze-out eccentricity of pions on collision energy in mid-central Au+Au collisions (E895, STAR) and Pb+Au collisions (CERES) for three rapidity regions and with ⟨$k_T$⟩ ≈ 0.31 GeV/c. Several (2+1)D hydrodynamical models and UrQMD calculations are shown. Model centralities correspond to the data.

The dependence of the kinetic freeze-out eccentricity of pions on collision energy in mid-central Au+Au collisions using UrQMD calculations, (2+1)D hydro MC-KLN and (2+1)D hydro MC-GLB models with ⟨$k_T$⟩ ≈ 0.31 GeV/c. Error bars include only statistical uncertainties. Model centralities correspond to the data.

The dependence of the kinetic freeze-out eccentricity of pions on collision energy in mid-central Au+Au collisions using (2+1)D hydro EOS-Q, (2+1)D hydro EOS-H, and (2+1)D hydro EOS-I models with ⟨$k_T$⟩ ≈ 0.31 GeV/c. Error bars include only statistical uncertainties. Model centralities correspond to the data.

Distribution of mT2 for events passing all the signal candidate selection requirements, except that on mT2 of the L100 selection, for DF events.

Distribution of mT2 for events passing all the signal candidate selection requirements, except that on mT2 of the L110 selection, for SF events.

Distribution of mT2 for events passing all the signal candidate selection requirements, except that on mT2 of the L110 selection, for DF events.

Observed 95% CL exclusion contour in the (STOP1, CHARGINO1) mass plane for a fixed value of m(NEUTRALINO1) = 1 GeV.

Expected 95% CL exclusion contour in the (STOP1, CHARGINO1) mass plane for a fixed value of m(NEUTRALINO1) = 1 GeV.

Observed 95% CL exclusion minus 1 sigma contour in the (STOP1, CHARGINO1) mass plane for a fixed value of m(NEUTRALINO1) = 1 GeV.

Observed 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane for a fixed value of m(STOP1) - m(CHARGINO1) = 10 GeV.

Expected 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane for a fixed value of m(STOP1) - m(CHARGINO1) = 10 GeV.

Observed 95% CL exclusion minus 1 sigma contour in the (STOP1, NEUTRALINO1) mass plane for a fixed value of m(STOP1) - m(CHARGINO1) = 10 GeV.

Observed 95% CL exclusion contour in the (CHARGINO1, NEUTRALINO1) mass plane for a fixed value of m(STOP1) = 300 GeV.

Expected 95% CL exclusion contour in the (CHARGINO1, NEUTRALINO1) mass plane for a fixed value of m(STOP1) = 300 GeV.

Observed 95% CL exclusion minus one sigma contour in the (CHARGINO1, NEUTRALINO1) mass plane for a fixed value of m(STOP1) = 300 GeV.

Observed 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane of m(CHARGINO1) = 2 m(NEUTRALINO1).

Expected 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane for m(CHARGINO1) = 2 m(NEUTRALINO1).

Observed 95% CL exclusion minus one sigma contour in the (STOP1, NEUTRALINO1) mass plane for m(CHARGINO1) = 2 m(NEUTRALINO1).

Observed 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane.

Expected 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane.

Observed 95% CL exclusion minus one sigma contour in the (STOP1, NEUTRALINO1) mass plane.

Observed 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane.

Expected 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane.

Observed 95% CL exclusion minus one sigma contour in the (STOP1, NEUTRALINO1) mass plane.

Observed 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane for a fixed value of m(CHARGINO1) = 106 GeV.

Expected 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane for a fixed value of m(CHARGINO1) = 106 GeV.

Observed 95% CL exclusion minus one sigma contour in the (STOP1, NEUTRALINO1) mass plane for a fixed value of m(CHARGINO1) = 106 GeV.

Expected CLs values for Fig. 14.

Observed CLs values for Fig. 14.

Observed cross-section limits for Fig. 14.

Expected CLs values for Fig. 15.

Observed CLs values for Fig. 15.

Observed cross-section limits for Fig. 15.

Expected CLs values for Fig. 16.

Observed CLs values for Fig. 16.

Observed cross-section limits for Fig. 14.

Expected CLs values for Fig. 17.

Observed CLs values for Fig. 17.

Observed cross-section limits for Fig. 17.

Expected CLs values for Fig. 19.

Observed CLs values for Fig. 19.

Observed cross-section limits for Fig. 19.

Number of generated events for Fig. 16.

Acceptance of S1 for Fig. 16.

Efficiency of S1 for Fig. 16.

Total systematic uncertainty IN PCT on signal yields in S1 for Fig. 16.

Acceptance of S2 for Fig. 16.

Efficiency of S2 for Fig. 16.

Total systematic uncertainty IN PCT on signal yields in S2 for Fig. 16.

Acceptance of S3 for Fig. 16.

Efficiency of S3 for Fig. 16.

Total systematic uncertainty IN PCT on signal yields in S3 for Fig. 16.

Acceptance of S4 for Fig. 16.

Efficiency of S4 for Fig. 16.

Total systematic uncertainty IN PCT on signal yields in S4 for Fig. 16.

Acceptance of S5 for Fig. 16.

Efficiency of S5 for Fig. 16.

Total systematic uncertainty IN PCT on signal yields in S5 for Fig. 16.

Acceptance of S6 for Fig. 16.

Efficiency of S6 for Fig. 16.

Total systematic uncertainty IN PCT on signal yields in S6 for Fig. 16.

Acceptance of S7 for Fig. 16.

Efficiency of S7 for Fig. 16.

Total systematic uncertainty IN PCT on signal yields in S7 for Fig. 16.

Acceptance of H160 for Fig. 16.

Efficiency of H160 for Fig. 16.

Total systematic uncertainty IN PCT on signal yields in H160 for Fig. 16.

Observed cross-section limits for Fig. 20.

Observed cross-section limits for Fig. 20.

Expected cross-section limits for Fig. 20.

Total number of generated MC events for each point of the grid.

Observed upper limit on the signal cross-section, in pb, for each point of the grid in the different flavour channel.

Observed upper limit on the signal cross-section, in pb, for each point of the grid in the same flavour channel.

The best expected signal region chosen for each point of the grid in the different flavour channel.

The best expected signal region chosen for each point of the grid in the same flavour channel.

Observed CLs for each point of the grid in the different flavour channel.

Observed CLs for each point of the grid in the same flavour channel.

Expected CLs for each point of the grid in the different flavour channel.

Expected CLs for each point of the grid in the same flavour channel.

Signal acceptance for all the analysis cuts, except the BDTG cut, for each point of the grid in the different flavour channel.

Signal acceptance for all the analysis cuts, except the BDTG cut, for each point of the grid in the same flavour channel.

Signal efficiency, including the acceptance of the BDTG cut, for each point of the grid in the different flavour channel.

Signal efficiency, including the acceptance of the BDTG cut, for each point of the grid in the same flavour channel.

Total signal experimental systematic uncertainty for each point of the grid in the different flavour channel.

Signal efficiency, including the acceptance of the BDTG cut, for each point of the grid in the same flavour channel.

Number of simulated events passing various stages of the selection in the hadronic mT2 analysis for a signal sample with m(STOP1)=300 GeV, m(CHARGINO1) = 150 GeV and m(NEUTRALINO1) = 50 GeV, and with the top squark decaying as STOP1 --> CHARGINO1+ BOTTOM -> W(*)+NEUTRALINO1+ BOTTOM with unit probability. Event weights are applied to correct simulated events to data. "Isolation" includes the effects of tight ID for electrons and the isolation selection for both electrons and muons. "Cleaning cuts" refer to cuts applied to remove non-collision backgrounds and detector noise.

Number of simulated events passing various stages of the selection in the hadronic mT2 analysis for a signal sample with m(STOP1)=250 GeV, m(CHARGINO1) = 106 GeV and m(NEUTRALINO1) = 60 GeV, and with the top squark decaying as STOP1 --> CHARGINO1+ BOTTOM -> W(*)+NEUTRALINO1+ BOTTOM with unit probability. Event weights are applied to correct simulated events to data. "Isolation" includes the effects of tight ID for electrons and the isolation selection for both electrons and muons. "Cleaning cuts" refer to cuts applied to remove non-collision backgrounds and detector noise.

Number of simulated events passing various stages of the selection in the leptonic mT2 analysis for two signal samples with the top squark decaying as STOP1 --> CHARGINO1+ BOTTOM -> W(*)+NEUTRALINO1+BOTTOM with unit probability. Event weights are applied to correct simulated events to data. "Isolation" includes the effects of tight ID for electrons and the isolation selection for both electrons and muons. "Cleaning cuts" refer to cuts applied to remove non-collision backgrounds and detector noise.

Number of simulated events passing various stages of the selection in the leptonic mT2 analysis for a signal sample with m(STOP1)=180 GeV and m(NEUTRALINO1) = 60 GeV, and with the top squark decaying as STOP1 --> W + BOTTOM + NEUTRALINO1 with unit probability. Event weights are applied to correct simulated events to data. "Isolation" includes the effects of tight ID for electrons and the isolation selection for both electrons and muons. "Cleaning cuts" refer to cuts applied to remove non-collision backgrounds and detector noise.

Number of simulated events passing various stages of the selection in the in the MVA analysis for all signal samples used to train the BDTG and with the top squark decaying as STOP1 --> TOP + NEUTRALINO1 with unit probability. Event weights are applied to correct simulated events to data. "Isolation" includes the effects of tight ID for electrons and the isolation selection for both electrons and muons. "Cleaning cuts" refer to cuts applied to remove non-collision backgrounds and detector noise. The index i in category (Ci) is the one reported in table 3 for each signal point, SF and DF.

Two-plane EP correlation from Glauber model from SP method and EP method.

Two-plane EP correlation data from SP method and EP method.

Two-plane EP correlation from Glauber model from SP method and EP method.

Two-plane EP correlation data from SP method and EP method.

Two-plane EP correlation from Glauber model from SP method and EP method.

Two-plane EP correlation data from SP method and EP method.

Two-plane EP correlation from Glauber model from SP method and EP method.

Two-plane EP correlation data from SP method and EP method.

Two-plane EP correlation from Glauber model from SP method and EP method.

Two-plane EP correlation data from SP method and EP method.

Two-plane EP correlation from Glauber model from SP method and EP method.

Two-plane EP correlation data from SP method and EP method.

Two-plane EP correlation from Glauber model from SP method and EP method.

Three-plane EP correlation data from SP method and EP method.

Three-plane EP correlation from Glauber model from SP method and EP method.

Three-plane EP correlation data from SP method and EP method.

Three-plane EP correlation from Glauber model from SP method and EP method.

Three-plane EP correlation data from SP method and EP method.

Three-plane EP correlation from Glauber model from SP method and EP method.

Three-plane EP correlation data from SP method and EP method.

Three-plane EP correlation from Glauber model from SP method and EP method.

Three-plane EP correlation data from SP method and EP method.

Three-plane EP correlation from Glauber model from SP method and EP method.

Three-plane EP correlation data from SP method and EP method.

Three-plane EP correlation from Glauber model from SP method and EP method.

For events in the low-ETmiss validation region, the M(l tau) distribution in VR1taua.

For events in the low-ETmiss validation region, the MT2max distribution in VR2taua.

For events in the high-ETmiss + b-tagged jet validation region, the ETmiss distribution in VR0taunoZb.

For events in the high-ETmiss + b-tagged jet validation region, the ETmiss distribution in VR0tauZb.

For events in the high-ETmiss + b-tagged jet validation region, the ETmiss distribution in VR1taub.

For events in the high-ETmiss + b-tagged jet validation region, the ETmiss distribution in VR2taub.

Expected distributions of SM background events and observed data distributions in the binned signal regions SR0taua.

The distribution of ETmiss in the summation of all SR0taua regions prior to the requirements on this variable.

The distribution of MT in the summation of all SR0taua regions prior to the requirements on this variable.

The distribution of M(SFOS) in the summation of all SR0taua regions prior to the requirements on this variable.

Expected distribution of SM background events and observed data distribution for the MIN(DELTA(PHI(ll))) variable in the SR0taub region, prior to the requirements on this variable.

Expected distribution of SM background events and observed data distribution for the ETmiss variable in the SR1tau region, prior to the requirements on this variable.

Expected distribution of SM background events and observed data distribution for the MT2max variable in the SR2taua region, prior to the requirements on this variable.

Expected distribution of SM background events and observed data distribution for the M(tau tau) variable in the SR2taub region, prior to the requirements on this variable.

Observed 95% CL exclusion contour for chargino and neutralino production in the sleptonL-mediated simplified model.

Expected 95% CL exclusion contour for chargino and neutralino production in the sleptonL-mediated simplified model.

Observed 95% CL exclusion contour for chargino and neutralino production in the WZ-mediated simplified model.

Expected 95% CL exclusion contour for chargino and neutralino production in the WZ-mediated simplified model.

Observed 95% CL exclusion contour for chargino and neutralino production in the stauL-mediated simplified model.

Expected 95% CL exclusion contour for chargino and neutralino production in the stauL-mediated simplified model.

Observed 95% CL exclusion contour for chargino and neutralino production in the Wh-mediated simplified model.

Expected 95% CL exclusion contour for chargino and neutralino production in the Wh-mediated simplified model.

Observed 95% CL exclusion contour in the pMSSM model with sleptons and M1 = 100 GeV.

Expected 95% CL exclusion contour in the pMSSM model with sleptons and M1 = 100 GeV.

Observed 95% CL exclusion contour in the pMSSM model with sleptons and M1 = 140 GeV.

Expected 95% CL exclusion contour in the pMSSM model with sleptons and M1 = 140 GeV.

Observed 95% CL exclusion contour in the pMSSM model with sleptons and M1 = 250 GeV.

Expected 95% CL exclusion contour in the pMSSM model with sleptons and M1 = 250 GeV.

Observed 95% CL exclusion contour in the pMSSM model with staus.

Expected 95% CL exclusion contour in the pMSSM model with staus.

Observed 95% CL exclusion contour in the pMSSM model with no sleptons.

Expected 95% CL exclusion contour in the pMSSM model with no sleptons.

Excluded model cross-sections at 95% confidence level for the slepL-mediated simplified model.

Excluded model cross-sections at 95% confidence level for WZ-mediated simplified model.

Excluded model cross-sections at 95% confidence level for stauL-mediated simplified model.

Excluded model cross-sections at 95% confidence level for Wh-mediated simplified model.

Number of generated signal events for slepL-mediated simplified model.

Number of generated signal events for WZ-mediated simplified model.

Number of generated signal events for stauL-mediated simplified model.

Number of generated signal events for Wh-mediated simplified model.

Cross-sections for slepL-mediated simplified model.

Cross-sections for WZ-mediated simplified model.

Cross-sections for stauL-mediated simplified model.

Cross-sections for Wh-mediated simplified model.

Acceptance for slepL-mediated simplified model using SR0taua bin 20.

Acceptance for WZ-mediated simplified model using SR0taua bin 16.

Acceptance for stauL-mediated simplified model using SR2taua.

Acceptance for Wh-mediated simplified model using SR2taub.

Efficiency for slepL-mediated simplified model using SR0taua bin 20.

Efficiency for WZ-mediated simplified model using SR0taua bin 16.

Efficiency for stauL-mediated simplified model using SR2taua.

Efficiency for Wh-mediated simplified model using SR2taub.

The total experimental uncertainty, not including Monte Carlo statistics, for the slepL-mediated simplified model using SR0taua bin 20.

The total experimental uncertainty, not including Monte Carlo statistics, for the WZ-mediated simplified model using SR0taua bin 16.

The total experimental uncertainty, not including Monte Carlo statistics, for the stauL-mediated simplified model using SR2taua.

The total experimental uncertainty, not including Monte Carlo statistics, for the Wh-mediated simplified model using SR2taub.

The expected CL for slepL-mediated simplified model using SR0taua bin 20, using pseudo-experiments.

The expected CL for WZ-mediated simplified model using SR0taua bin 16, using pseudo-experiments.

The expected CL for stauL-mediated simplified model using SR2taua, using pseudo-experiments.

The expected CL for Wh-mediated simplified model using SR2taub, using pseudo-experiments.

The observed CL for slepL-mediated simplified model using SR0taua bin 20, using pseudo-experiments.

The observed CL for WZ-mediated simplified model using SR0taua bin 16, using pseudo-experiments.

The observed CL for stauL-mediated simplified model using SR2taua, using pseudo-experiments.

The observed CL for Wh-mediated simplified model using SR2taub, using pseudo-experiments.

Measured differential cross sections as function of the lepton pseudo-rapidity of the production of a W boson with a D meson or a D* meson times the branching ratio W -> l nu in the fiducial regions together with the statistical and systematic uncertainties. Jets are not required for the W+D/D* cross sections. The cross sections are defined for OS-SS events.

Measured cross section ratios of the production of a W boson with a D meson or a D* meson and the inclusive production of a W boson in the fiducial regions together with the statistical and systematic uncertainties. Jets are not required for the W+D/D* cross sections. The cross sections are defined for OS-SS events.

Measured differential cross section ratios of the production of a W boson with a D meson or a D* meson and the inclusive production of a W boson in the fiducial regions as function of the D/D* meson pT together with the statistical and systematic uncertainties. Jets are not required for the W+D/D* cross sections. The cross sections are defined for OS-SS events.

Measured integrated cross sections of the production of a W boson in association with a single c-jet and exactly zero or one additional non-c-jets times the branching ratio W -> l nu in the fiducial regions together with the statistical and systematic uncertainties. The particle-level c-jet is defined as the one containing a weakly decaying c-hadron with pt>5 GeV, within DeltaR<0.3. Jets containing c-hadrons originating from b-hadron decays are not counted as c-jets. The cross sections are defined for OS-SS events.

Measured integrated cross sections ratio of the production of a W+ and W- bosons in association with a single c-jet and exactly zero or one additional non-c-jets in the fiducial regions together with the statistical and systematic uncertainties. The particle-level c-jet is defined as the one containing a weakly decaying c-hadron with pt>5 GeV, within DeltaR<0.3. Jets containing c-hadrons originating from b-hadron decays are not counted as c-jets. The cross sections are defined for OS-SS events.

Measured integrated cross sections of the production of a W boson in association with a single c-jet decaying into a soft muon in the fiducial regions together with the statistical and systematic uncertainties. The particle-level c-jet is defined as the one containing a weakly decaying c-hadron with pt>5 GeV, within DeltaR<0.3. Jets containing c-hadrons originating from b-hadron decays are not counted as c-jets. Soft muons are associated to c-jets within a cone of DeltaR<0.5. Jets are not required for the W+D/D* cross sections. The cross sections are defined for OS-SS events.

Correlation matrix corresponding to the total uncertainties of measured integrated cross sections of the production of a W boson with a single c-jet, a D meson or a D* meson times the branching ratio W -> l nu in the fiducial regions.

Systematic uncertainties after the averaging procedure of the inclusive cross sections in different channels. The first row (labeled Uncorr.) represents the uncorrelated systematic uncertainties. The following rows represent the diagonalized list of systematic uncertainties which are correlated across all channels. The luminosity is included in these correlated systematic uncertainties.

Systematic uncertainties after the averaging procedure of the differential cross sections as function of the lepton pseudo-rapidity in different channels. The first row (labeled Uncorr.) represents the uncorrelated systematic uncertainties. The following rows represent the diagonalized list of systematic uncertainties which are correlated across all channels and bins. The luminosity is included in these correlated systematic uncertainties. The systematic uncertainties for the W+ + cbar-jet channel are shown in this table.

Systematic uncertainties after the averaging procedure of the differential cross sections as function of the lepton pseudo-rapidity in different channels. The first row (labeled Uncorr.) represents the uncorrelated systematic uncertainties. The following rows represent the diagonalized list of systematic uncertainties which are correlated across all channels and bins. The luminosity is included in these correlated systematic uncertainties. The systematic uncertainties for the W- + c-jet channel are shown in this table.

Systematic uncertainties after the averaging procedure of the differential cross sections as function of the lepton pseudo-rapidity in different channels. The first row (labeled Uncorr.) represents the uncorrelated systematic uncertainties. The following rows represent the diagonalized list of systematic uncertainties which are correlated across all channels and bins. The luminosity is included in these correlated systematic uncertainties. The systematic uncertainties for the W+ D- and W- D+ channels are shown in this table.

Systematic uncertainties after the averaging procedure of the differential cross sections as function of the lepton pseudo-rapidity in different channels. The first row (labeled Uncorr.) represents the uncorrelated systematic uncertainties. The following rows represent the diagonalized list of systematic uncertainties which are correlated across all channels and bins. The luminosity is included in these correlated systematic uncertainties. The systematic uncertainties for the W+ D*- and W- D*+ channels are shown in this table.

Theoretical Predictions for the integrated cross section of the production of W+ and W- bosons associated with a single c-jet, a D meson or a D* meson in the fiducial regions together with the statistical and systematic uncertainties. For the W+c-jet cross sections events with more than one c-jet are discarded. The particle-level c-jet is defined as the one containing a weakly decaying c-hadron with pt>5 GeV, within DeltaR<0.3. Jets containing c-hadrons originating from b-hadron decays are not counted as c-jets. Jets are not required for the W+D/D* cross sections. The cross sections are defined for OS-SS events. The predictions have been obtained the aMC@NLO MC simulation interfaced to the Herwig++ parton shower programme. The uncertainties on the predictions entail PDF uncertainties, parton shower, fragmentation and scale uncertainties. The predictions are reweighted using LHAPDF from the CT10nlo PDF set to the following PDF sets with the LHAPDF IDs given in brackets: CT10nlo (11000), MSTW2008nlo68cl (21100), NNPDF23_nlo_as_0119 (230000), NNPDF23_nlo_collider_as_0119 (236000), HERAPDF15NLO (EIG+VAR, 60700+60730), ATLAS-epWZ12 (EIG+VAR, 65000+65040).

PDF uncertainty for each of the used PDF sets as well as the combined parton shower, fragmentation and scale uncertainties (given in percent) for the theoretical Predictions for the integrated cross section of the production of W+ and W- bosons associated with a single c-jet, a D meson or a D* meson in the fiducial regions together with the statistical and systematic uncertainties. If added quadratically, these uncertainties represent the total uncertainty on the quoted theory prediction. For the W+c-jet cross sections events with more than one c-jet are discarded. The particle-level c-jet is defined as the one containing a weakly decaying c-hadron with pt>5 GeV, within DeltaR<0.3. Jets containing c-hadrons originating from b-hadron decays are not counted as c-jets. Jets are not required for the W+D/D* cross sections. The cross sections are defined for OS-SS events. The predictions have been obtained the aMC@NLO MC simulation interfaced to the Herwig++ parton shower programme. The uncertainties on the predictions entail PDF uncertainties, FSR uncertainties and scale uncertainties. The predictions are reweighted using LHAPDF from the CT10nlo PDF set to the following PDF sets with the LHAPDF IDs given in brackets: CT10nlo (11000), MSTW2008nlo68cl (21100), NNPDF23_nlo_as_0119 (230000), NNPDF23_nlo_collider_as_0119 (236000), HERAPDF15NLO (EIG+VAR, 60700+60730), ATLAS-epWZ12 (EIG+VAR, 65000+65040). The determination of the parton shower, fragmentation and scale uncertainties is detailed in the paper.

The dielectron $v_2$ as a function of $p_T$ in minimum-bias Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV for the $\eta$ mass region.

The dielectron $v_2$ as a function of $p_T$ in minimum-bias Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV for the charm + $ ho^0$ mass region.

The dielectron $v_2$ as a function of $p_T$ in minimum-bias Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV for the $\omega$ mass region.

The dielectron $v_2$ as a function of $p_T$ in minimum-bias Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV for the $\phi$ mass region.

The dielectron $v_2$ as a function of $p_T$ in minimum-bias Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV for the charm + thermal radiation mass region.

The dielectron $v_2$ as a function of $p_T$ in minimum-bias Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV expected from decays of a mesonic cocktail.

The dielectron $v_2$ as a function of $p_T$ in minimum-bias Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV expected from decays of a mesonic cocktail.

The dielectron $v_2$ as a function of $p_T$ in minimum-bias Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV expected from decays of a mesonic cocktail.

The dielectron $v_2$ as a function of $p_T$ in minimum-bias Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV expected from decays of a mesonic cocktail.

The dielectron $v_2$ as a function of $p_T$ in minimum-bias Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV expected from decays of a mesonic cocktail.

The dielectron $v_2$ as a function of $p_T$ in minimum-bias Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV expected from the $car{c}$ contribution.

The $p_T$-integrated dielectron $v_2$ as a function of $M_{ee}$ in minimum-bias Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

The $v_2$ of hadrons $\pi$, $K$, $p$, $\phi$ and $\Lambda$ in minimum-bias Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV for the $\pi^0$ mass region.

The $p_T$-integrated dielectron $v_2$ as a function of $M_{ee}$ in minimum-bias Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV, expected from the decays of $\pi^0$, $\eta$, $\omega$ and $\phi$ and from the $car{c}$ contribution.

The efficiency and centrality bin width corrected mean (M) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 27 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected mean (M) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 39 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected mean (M) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 62.4 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected mean (M) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 200 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected standard deviation ($\sigma$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 7.7 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected standard deviation ($\sigma$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 11.5 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected standard deviation ($\sigma$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 19.6 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected standard deviation ($\sigma$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 27 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected standard deviation ($\sigma$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 39 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected standard deviation ($\sigma$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 62.4 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected standard deviation ($\sigma$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 200 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected skewness ($S$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 7.7 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected skewness ($S$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 11.5 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected skewness ($S$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 19.6 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected skewness ($S$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 27 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected skewness ($S$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 39 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected skewness ($S$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 62.4 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected skewness ($S$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 200 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected kurtosis ($\kappa$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 7.7 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected kurtosis ($\kappa$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 11.5 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected kurtosis ($\kappa$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 19.6 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected kurtosis ($\kappa$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 27 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected kurtosis ($\kappa$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 39 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected kurtosis ($\kappa$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 62.4 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected kurtosis ($\kappa$) of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 200 GeV. The dotted lines represent calculations from the central limit theorem. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected $S\sigma$ of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 7.7 GeV. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected $S\sigma$ of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 11.5 GeV. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected $S\sigma$ of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 19.6 GeV. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected $S\sigma$ of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 27 GeV. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected $S\sigma$ of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 39 GeV. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected $S\sigma$ of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 62.4 GeV. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected $S\sigma$ of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 200 GeV. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected $\kappa\sigma^2$ of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 7.7 GeV. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected $\kappa\sigma^2$ of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 11.5 GeV. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected $\kappa\sigma^2$ of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 19.6 GeV. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected $\kappa\sigma^2$ of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 27 GeV. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected $\kappa\sigma^2$ of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 39 GeV. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected $\kappa\sigma^2$ of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 62.4 GeV. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected $\kappa\sigma^2$ of the net-charge multiplicity distributions as a function of number of participating nucleons $N_{part}$ for Au+Au collisions at 200 GeV. The error bars are statisticaland systematic errors.

The efficiency and centrality bin width corrected $\sigma^2/M$ of the net-charge multiplicity distributions as a function of collision energy for Au+Au collisions. The error bars are statistical and the caps represent systematic errors.

The efficiency and centrality bin width corrected $S\sigma^2$ of the net-charge multiplicity distributions as a function of collision energy for Au+Au collisions. The error bars are statistical and the caps represent systematic errors.

The efficiency and centrality bin width corrected $\kappa\sigma^2$ of the net-charge multiplicity distributions as a function of collision energy for Au+Au collisions. The error bars are statistical and the caps represent systematic errors.