The TPC mid-rapidity multiplicity distributions ($|\eta|$ < 0.5) for the corresponding E-FTPC selected centrality bins.

Uncorrected charged particle multiplicity distribution measured in the TPC within $|\eta|$ < 0.5 in pp collisions at 200 GeV.

The ratio of the transverse overlap area $S_{⊥}$ to $(N_{part}/2)^{2/3}$ versus $(N_{part}/2)^{2/3}$.

The ratio of the transverse overlap area $S_{⊥}$ to $(N_{part}/2)^{2/3}$ versus $(N_{part}/2)^{2/3}$.

The ratio of the transverse overlap area $S_{⊥}$ to $(N_{part}/2)^{2/3}$ versus $(N_{part}/2)^{2/3}$.

The ratio of the charged pion multiplicity to the transverse overlap area $dN_{\pi}/dy/S_{⊥}$ versus $N_{coll}/N_{part}$. Errors shown are total errors, dominated by systematic uncertainties. The systematic uncertainties are correlated between Npart, Ncoll, and S⊥, and are largely canceled in the plotted ratio quantities.

The ratio of the charged pion multiplicity to the transverse overlap area $dN_{\pi}/dy/S_{⊥}$ versus $N_{coll}/N_{part}$. Errors shown are total errors, dominated by systematic uncertainties. The systematic uncertainties are correlated between Npart, Ncoll, and S⊥, and are largely canceled in the plotted ratio quantities.

The ratio of the charged pion multiplicity to the transverse overlap area $dN_{\pi}/dy/S_{⊥}$ versus $N_{coll}/N_{part}$. Errors shown are total errors, dominated by systematic uncertainties. The systematic uncertainties are correlated between Npart, Ncoll, and S⊥, and are largely canceled in the plotted ratio quantities.

Energy loss effect for $\pi^{+-}$ (a), $K^{+-}$ (b), and p and pbar (c) at mid-rapidity (|y| < 0.1) as a function of particle momentum magnitude in 200 GeV pp and 62.4 GeV central 0-5% Au+Au collisions. Only negative particles are shown; energy loss for particles and antiparticles are the same. Errors shown are statistical only. The pion energy loss is already corrected by the track reconstruction algorithm.

Energy loss effect for $\pi^{+-}$ (a), $K^{+-}$ (b), and p and pbar (c) at mid-rapidity (|y| < 0.1) as a function of particle momentum magnitude in 200 GeV pp and 62.4 GeV central 0-5% Au+Au collisions. Only negative particles are shown; energy loss for particles and antiparticles are the same. Errors shown are statistical only. The pion energy loss is already corrected by the track reconstruction algorithm.

Energy loss effect for $\pi^{+-}$ (a), $K^{+-}$ (b), and p and pbar (c) at mid-rapidity (|y| < 0.1) as a function of particle momentum magnitude in 200 GeV pp and 62.4 GeV central 0-5% Au+Au collisions. Only negative particles are shown; energy loss for particles and antiparticles are the same. Errors shown are statistical only. The pion energy loss is already corrected by the track reconstruction algorithm.

Vertex-finding efficiency (ǫvtx) and fake vertex rate (δfake) as a function of the number of good global tracks (a) and the number of good primary tracks (b). Errors shown or smaller than the point size are statistical only.

Vertex-finding efficiency (ǫvtx) and fake vertex rate (δfake) as a function of the number of good global tracks (a) and the number of good primary tracks (b). Errors shown or smaller than the point size are statistical only.

The $p_{T}$ dependent correction to particle spectra due to fake vertex events, $\epsilon_{fake}(p_{T})$, in 200 GeV minimum bias pp and d+Au collisions. Errors shown are statistical only.

The $p_{T}$ dependent correction to particle spectra due to fake vertex events, $\epsilon_{fake}(p_{T})$, in 200 GeV minimum bias pp and d+Au collisions. Errors shown are statistical only.

Efficiency (product of tracking efficiency and detector acceptance) of π−, K−, and p in pp (a) and d+Au collisions (b) at 200 GeV as a function of input MC p⊥. Errors shown are binomial errors. The curves are parameterizations to the efficiency data and are used for corrections in the analysis.

Efficiency (product of tracking efficiency and detector acceptance) of π−, K−, and p in pp (a) and d+Au collisions (b) at 200 GeV as a function of input MC p⊥. Errors shown are binomial errors. The curves are parameterizations to the efficiency data and are used for corrections in the analysis.

Efficiency (product of tracking efficiency and detector acceptance) of π−, K−, and p in 70-80% peripheral Au+Au (a) and 0-5% central Au+Au collisions (b) at 62.4 GeV as a function of input MC p⊥. Errors shown are binomial errors. The curves are parameterizations to the efficiency data and are used for corrections in the analysis.

Efficiency (product of tracking efficiency and detector acceptance) of π−, K−, and p in 70-80% peripheral Au+Au (a) and 0-5% central Au+Au collisions (b) at 62.4 GeV as a function of input MC p⊥. Errors shown are binomial errors. The curves are parameterizations to the efficiency data and are used for corrections in the analysis.

Efficiency (product of tracking efficiency and detector acceptance) of π−, K−, and p in 70-80% peripheral Au+Au (a) and 0-5% central Au+Au collisions (b) at 62.4 GeV as a function of input MC p⊥. Errors shown are binomial errors. The curves are parameterizations to the efficiency data and are used for corrections in the analysis.

Efficiency (product of tracking efficiency and detector acceptance) of π−, K−, and p in 70-80% peripheral Au+Au (a) and 0-5% central Au+Au collisions (b) at 62.4 GeV as a function of input MC p⊥. Errors shown are binomial errors. The curves are parameterizations to the efficiency data and are used for corrections in the analysis.

The dca distributions of protons and antiprotons for 0.40 < p⊥ < 0.45 GeV/c in 200 GeV minimum bias d+Au. Errors shown are statistical only.

The dca distributions of protons and antiprotons for 0.70 < p⊥ < 0.75 GeV/c in 200 GeV minimum bias d+Au. Errors shown are statistical only.

The dca distributions of protons and antiprotons for 0.40 < p⊥ < 0.45 GeV/c in 62.4 GeV 0-5% central Au+Au collisions. Errors shown are statistical only.

The dca distributions of protons and antiprotons for 0.70 < p⊥ < 0.75 GeV/c in 62.4 GeV 0-5% central Au+Au collisions. Errors shown are statistical only.

Pion background fraction from weak decays ($\Lambda, K_S^0$) and $\mu^{+-}$ contamination as a function of p⊥ in minimum bias d+Au collisions at 200 GeV. Errors shown are statistical only.

Pion background fraction from weak decays ($\Lambda, K_S^0$) and $\mu^{+-}$ contamination as a function of p⊥ in minimum bias d+Au collisions at 200 GeV. Errors shown are statistical only.

Mid-rapidity identified antiproton spectra in 200 GeV minimum bias d+Au (a) and 62.4 GeV central Au+Au collisions (b) measured by dE/dx together with those by TOF [46, 47]. The dE/dx data are from |y| < 0.1 and the TOF data are from |y| < 0.5. The curves are various fits to the dE/dx data for extrapolation. The quadratic sum of statistical errors and point-to-point systematic errors are plotted, but are smaller than the point size.

Mid-rapidity identified antiproton spectra in 200 GeV minimum bias d+Au (a) and 62.4 GeV central Au+Au collisions (b) measured by dE/dx together with those by TOF [46, 47]. The dE/dx data are from |y| < 0.1 and the TOF data are from |y| < 0.5. The curves are various fits to the dE/dx data for extrapolation. The quadratic sum of statistical errors and point-to-point systematic errors are plotted, but are smaller than the point size.

Mid-rapidity identified antiproton spectra in 200 GeV minimum bias d+Au (a) and 62.4 GeV central Au+Au collisions (b) measured by dE/dx together with those by TOF [46, 47]. The dE/dx data are from |y| < 0.1 and the TOF data are from |y| < 0.5. The curves are various fits to the dE/dx data for extrapolation. The quadratic sum of statistical errors and point-to-point systematic errors are plotted, but are smaller than the point size.

Mid-rapidity identified antiproton spectra in 200 GeV minimum bias d+Au (a) and 62.4 GeV central Au+Au collisions (b) measured by dE/dx together with those by TOF [46, 47]. The dE/dx data are from |y| < 0.1 and the TOF data are from |y| < 0.5. The curves are various fits to the dE/dx data for extrapolation. The quadratic sum of statistical errors and point-to-point systematic errors are plotted, but are smaller than the point size.

Mid-rapidity identified antiproton spectra in 200 GeV minimum bias d+Au (a) and 62.4 GeV central Au+Au collisions (b) measured by dE/dx together with those by TOF [46, 47]. The dE/dx data are from |y| < 0.1 and the TOF data are from |y| < 0.5. The curves are various fits to the dE/dx data for extrapolation. The quadratic sum of statistical errors and point-to-point systematic errors are plotted, but are smaller than the point size.

Mid-rapidity identified antiproton spectra in 200 GeV minimum bias d+Au (a) and 62.4 GeV central Au+Au collisions (b) measured by dE/dx together with those by TOF [46, 47]. The dE/dx data are from |y| < 0.1 and the TOF data are from |y| < 0.5. The curves are various fits to the dE/dx data for extrapolation. The quadratic sum of statistical errors and point-to-point systematic errors are plotted, but are smaller than the point size.

Mid-rapidity identified antiproton spectra in 200 GeV minimum bias d+Au (a) and 62.4 GeV central Au+Au collisions (b) measured by dE/dx together with those by TOF [46, 47]. The dE/dx data are from |y| < 0.1 and the TOF data are from |y| < 0.5. The curves are various fits to the dE/dx data for extrapolation. The quadratic sum of statistical errors and point-to-point systematic errors are plotted, but are smaller than the point size.

Mid-rapidity identified antiproton spectra in 200 GeV minimum bias d+Au (a) and 62.4 GeV central Au+Au collisions (b) measured by dE/dx together with those by TOF [46, 47]. The dE/dx data are from |y| < 0.1 and the TOF data are from |y| < 0.5. The curves are various fits to the dE/dx data for extrapolation. The quadratic sum of statistical errors and point-to-point systematic errors are plotted, but are smaller than the point size.

Mid-rapidity identified antiproton spectra in 200 GeV minimum bias d+Au (a) and 62.4 GeV central Au+Au collisions (b) measured by dE/dx together with those by TOF [46, 47]. The dE/dx data are from |y| < 0.1 and the TOF data are from |y| < 0.5. The curves are various fits to the dE/dx data for extrapolation. The quadratic sum of statistical errors and point-to-point systematic errors are plotted, but are smaller than the point size.

Mid-rapidity identified antiproton spectra in 200 GeV minimum bias d+Au (a) and 62.4 GeV central Au+Au collisions (b) measured by dE/dx together with those by TOF [46, 47]. The dE/dx data are from |y| < 0.1 and the TOF data are from |y| < 0.5. The curves are various fits to the dE/dx data for extrapolation. The quadratic sum of statistical errors and point-to-point systematic errors are plotted, but are smaller than the point size.

Mid-rapidity (|y| < 0.1) identified particle spectra in d+Au collisions at 200 GeV. The p and pbar spectra are inclusive, including weak decay products. Spectra are plotted for three centrality bins and for minimum bias events. Spectra from top to bottom are for 0-20% scaled by 4, 20-40% scaled by 2, minimum bias not scaled, and 40-100% scaled by 1/2. Errors plotted are statistical and point-to-point systematic errors added in quadrature, but are smaller than the point size. The curves are the blast-wave model fits to the minimum bias data; the normalizations of the curves are fixed by the corresponding negative particle spectra.

Mid-rapidity (|y| < 0.1) identified particle spectra in d+Au collisions at 200 GeV. The p and pbar spectra are inclusive, including weak decay products. Spectra are plotted for three centrality bins and for minimum bias events. Spectra from top to bottom are for 0-20% scaled by 4, 20-40% scaled by 2, minimum bias not scaled, and 40-100% scaled by 1/2. Errors plotted are statistical and point-to-point systematic errors added in quadrature, but are smaller than the point size. The curves are the blast-wave model fits to the minimum bias data; the normalizations of the curves are fixed by the corresponding negative particle spectra.

Mid-rapidity (|y| < 0.1) identified particle spectra in d+Au collisions at 200 GeV. The p and pbar spectra are inclusive, including weak decay products. Spectra are plotted for three centrality bins and for minimum bias events. Spectra from top to bottom are for 0-20% scaled by 4, 20-40% scaled by 2, minimum bias not scaled, and 40-100% scaled by 1/2. Errors plotted are statistical and point-to-point systematic errors added in quadrature, but are smaller than the point size. The curves are the blast-wave model fits to the minimum bias data; the normalizations of the curves are fixed by the corresponding negative particle spectra.

Mid-rapidity (|y| < 0.1) identified particle spectra in Au+Au collisions at 62.4 GeV. The p and p spectra are inclusive, including weak decay products. Spectra are plotted for nine centrality bins, from top to bottom, 0-5%, 5-10%, 10-20%, 20-30%, 30-40%, 40-50%, 50-60%, 60-70%, and 70-80%. Errors plotted are statistical and point-to-point systematic errors added in quadrature, but are smaller than the point size. The curves are the blast-wave model fits to the spectra; the normalizations of the curves in (a,b) are fixed by the corresponding negative particle spectra.

Mid-rapidity (|y| < 0.1) identified particle spectra in Au+Au collisions at 62.4 GeV. The p and p spectra are inclusive, including weak decay products. Spectra are plotted for nine centrality bins, from top to bottom, 0-5%, 5-10%, 10-20%, 20-30%, 30-40%, 40-50%, 50-60%, 60-70%, and 70-80%. Errors plotted are statistical and point-to-point systematic errors added in quadrature, but are smaller than the point size. The curves are the blast-wave model fits to the spectra; the normalizations of the curves in (a,b) are fixed by the corresponding negative particle spectra.

Mid-rapidity (|y| < 0.1) identified particle spectra in Au+Au collisions at 62.4 GeV. The p and p spectra are inclusive, including weak decay products. Spectra are plotted for nine centrality bins, from top to bottom, 0-5%, 5-10%, 10-20%, 20-30%, 30-40%, 40-50%, 50-60%, 60-70%, and 70-80%. Errors plotted are statistical and point-to-point systematic errors added in quadrature, but are smaller than the point size. The curves are the blast-wave model fits to the spectra; the normalizations of the curves in (a,b) are fixed by the corresponding negative particle spectra.

Mid-rapidity (|y| < 0.1) identified particle spectra in Au+Au collisions at 62.4 GeV. The p and p spectra are inclusive, including weak decay products. Spectra are plotted for nine centrality bins, from top to bottom, 0-5%, 5-10%, 10-20%, 20-30%, 30-40%, 40-50%, 50-60%, 60-70%, and 70-80%. Errors plotted are statistical and point-to-point systematic errors added in quadrature, but are smaller than the point size. The curves are the blast-wave model fits to the spectra; the normalizations of the curves in (a,b) are fixed by the corresponding negative particle spectra.

Mid-rapidity (|y| < 0.1) identified pion spectra in Au+Au collisions at 130 GeV. Spectra are plotted for eight centrality bins, from top to bottom, 0-6%, 6-11%, 11-18%, 18- 26%, 26-34%, 34-45%, 45-58%, and 58-85%. Errors plotted are statistical and point-to-point systematic errors added in quadrature, but they are smaller than the data point size. The curves are the Bose-Einstein fits to the spectra; the normalizations of the curves are fixed by the corresponding negative particle spectra.

Estimate of the product of the Bjorken energy density and the formation time ($\epsilon_{B_j}\tau$) as a function of centrality Npart. Errors shown are the quadratic sum of statistical and systematic uncertainties.

Estimate of the product of the Bjorken energy density and the formation time ($\epsilon_{B_j}\tau$) as a function of centrality Npart. Errors shown are the quadratic sum of statistical and systematic uncertainties.

Estimate of the product of the Bjorken energy density and the formation time ($\epsilon_{B_j}\tau$) as a function of centrality Npart. Errors shown are the quadratic sum of statistical and systematic uncertainties.

The K+/π+ and K−/π− ratios as a function of the collision energy in pp and central heavy-ion collisions.

The K+/K− ratio as a function of the collision energy in central heavy-ion collisions.

The K−/π− ratio as a function of the number of participants Npart in heavy-ion collisions at RHIC. Errors shown are the quadratic sum of statistical and systematic uncertainties.

The K−/π− ratio as a function of the number of participants Npart in heavy-ion collisions at RHIC. Errors shown are the quadratic sum of statistical and systematic uncertainties.

The K−/π− ratio as a function of the number of participants Npart in heavy-ion collisions at RHIC. Errors shown are the quadratic sum of statistical and systematic uncertainties.

The K−/π− ratio as a function of dNπ/dy/S⊥ in heavy-ion collisions at RHIC. Errors shown are the quadratic sum of statistical and systematic uncertainties.

The K−/π− ratio as a function of dNπ/dy/S⊥ in heavy-ion collisions at RHIC. Errors shown are the quadratic sum of statistical and systematic uncertainties.

The K−/π− ratio as a function of dNπ/dy/S⊥ in heavy-ion collisions at RHIC. Errors shown are the quadratic sum of statistical and systematic uncertainties.

Baryon chemical potential extracted for central heavy-ion collisions as a function of the collision energy. Errors shown are the total statistical and systematic errors.

The extracted chemical freeze-out temperatures for central heavy-ion collisions as a function of the collision energy. Errors shown are the total statistical and systematic errors.

The extracted chemical freeze-out temperatures for central heavy-ion collisions as a function of the collision energy. Errors shown are the total statistical and systematic errors.

The extracted kinetic freeze-out temperatures for central heavy-ion collisions as a function of the collision energy. Errors shown are the total statistical and systematic errors.

Average transverse radial flow velocity extracted from the blast-wave model for central heavy-ion collisions as a function of the collision energy. Errors shown are the total statistical and systematic errors.

Phase diagram plot of chemical freezeout temperature versus baryon chemical potential extracted from chemical equilibrium models. Errors shown are the total statistical and systematic errors.

Phase diagram plot of chemical freezeout temperature versus baryon chemical potential extracted from chemical equilibrium models. Errors shown are the total statistical and systematic errors.

Differential cross-sections obtained from the optical and MC Glauber calculations for Au+Au collisions at 200 GeV. Statistical errors are smaller than the point size.

Differential cross-sections obtained from the optical and MC Glauber calculations for Au+Au collisions at 200 GeV. Statistical errors are smaller than the point size.

Distribution of the total energy outside the reconstructed jets for the completed data samples. Also tabulated is the estimated background.

Distribution of the total energy outside the reconstructed jets for the 'Dir' domain. Also tabulated is the estimated background.

Distribution of the total energy outside the reconstructed jets for the 'SR' domain. Also tabulated is the estimated background.

Distribution of the total energy outside the reconstructed jets for the 'DR' domain. Also tabulated is the estimated background.

Observed distribution of the charged particle multiplicity.

Observed distribution of the charged particle invariant mass.

Observed distribution of the mean of X(C=GAMMA-PLUS) and X(GAMMA-MINUS).

Observed mean number of particles in the reconstructed jets.

PHI transverse momentum spectra at incident energy 80 GeV/nucleon integrated over the rapidity range 0 to 1.7.

PHI transverse momentum spectra at incident energy 158 GeV/nucleon integrated over the rapidity range 0 to 1.0.

PHI transverse mass spectra at incident energy 20 GeV/nucleon integrated over the rapidity range 0 to 1.8.

PHI transverse mass spectra at incident energy 30 GeV/nucleon integrated over the rapidity range 0 to 1.8.

PHI transverse mass spectra at incident energy 40 GeV/nucleon integrated over the rapidity range 0 to 1.5.

PHI transverse mass spectra at incident energy 80 GeV/nucleon integrated over the rapidity range 0 to 1.7.

PHI transverse mass spectra at incident energy 158 GeV/nucleon integrated over the rapidity range 0 to 1.0.

Slope parameter as a function of rapidity for incident energy 158 GeV/nucleon. Here slope is defined as :-. DN/DPT = CONST*PT*EXP(-MT/SLOPE).

PHI rapidity distributions for incident energy 20 GeV/nucleon.

PHI rapidity distributions for incident energy 30 GeV/nucleon.

PHI rapidity distributions for incident energy 40 GeV/nucleon.

PHI rapidity distributions for incident energy 80 GeV/nucleon.

PHI rapidity distributions for incident energy 158 GeV/nucleon.

PHI/PI ratio extrapolated to final phase space.

PHI/PI ratio at mid rapidity.

PHI multiplicity.

Values of slope parameter, mean PT and mean MT as a function of energy.

Multiplicity distributions measured in the current region of the Breit frame for the bin of 2*E(Breit,current region) = 12 to 20.

Multiplicity distributions measured in the current region of the Breit frame for the bin of 2*E(Breit,current region) = 20 to 30.

Multiplicity distributions measured in the current region of the Breit frame for the bin of 2*E(Breit,current region) = 30 to 45.

Multiplicity distributions measured in the current region of the Breit frame for the bin of 2*E(Breit,current region) = 45 to 100.

Multiplicity distributions measured in the current region of the Breit frame for the Meff bin 1.5 to 4.

Multiplicity distributions measured in the current region of the Breit frame for the Meff bin 4 to 8.

Multiplicity distributions measured in the current region of the Breit frame for the Meff bin 8 to 12.

Multiplicity distributions measured in the current region of the Breit frame for the Meff bin 12 to 20.

Multiplicity distributions measured in the current region of the hadronic centre of mass (HCM) frame for W = 70 to 100 GeV.

Multiplicity distributions measured in the current region of the hadronic centre of mass (HCM) frame for W = 100 to 150 GeV.

Multiplicity distributions measured in the current region of the hadronic centre of mass (HCM) frame for W = 150 to 225 GeV.

Multiplicity distributions measured in the current region of the hadronic centre of mass (HCM) frame for the Meff bin 1.5 to 4.

Multiplicity distributions measured in the current region of the hadronic centre of mass (HCM) frame for the Meff bin 4 to 8.

Multiplicity distributions measured in the current region of the hadronic centre of mass (HCM) frame for the Meff bin 8 to 12.

Multiplicity distributions measured in the current region of the hadronic centre of mass (HCM) frame for the Meff bin 12 to 20.

Multiplicity distributions measured in the current region of the hadronic centre of mass (HCM) frame for the Meff bin 20 to 30.

Mean charged multiplicity measured in the Breit frame as a function of 2*E(Breit current region) with the assumptions of stable or decaying K0 and LAMBDA particles.

Mean charged multiplicity measured to the current fragmentation region of the HCM frame as a function of W with the assumptions of stable or decaying K0 and LAMBDA particles.

Mean charged multiplicity measured in the Breit frame as a function of Meff with the assumptions of stable or decaying K0 and LAMBDA particles.

Mean charged multiplicity measured in the current fragmentation region of the HCM frame as a function of Meff with the assumptions of stable or decaying K0 and LAMBDA particles.

Transverse mass spectra for kaon production in the central rapidity region for collisions at 20 GeV per nucleon.

Transverse mass spectra for kaon production in the central rapidity region for collisions at 30 GeV per nucleon.

Rapidity distribution of PI- production.

Rapidity distribution of K- production.

Rapidity distribution of K+ production.

Energy dependence of the mean K+ to PI+ and K- to PI- multiplicity ratio with the full phase space.. The data below 6 GeV are from the AGS and above 100 GeV from RHIC.

Energy dependence of the mean K+ to PI+ and K- to PI- multiplicity ratio mid rapidity regions.. The data below 6 GeV are from the AGS and above 100 GeV from RHIC.

Energy dependence of the inverse slope parameter of the transverse mass spectra in K+ and K- production.. The data below 6 GeV are from the AGS and above 100 GeV from RHIC.

Energy dependence of the mean transverse mass measured at mid rapidity in PI+ and PI- production.. The data below 6 GeV are from the AGS and above 100 GeV from RHIC.

Energy dependence of the mean transverse mass measured at mid rapidity in K+ and K- production.. The data below 6 GeV are from the AGS and above 100 GeV from RHIC.

Normalised distribution of the scaled momentum as a function of Q**2 in the X range 0.02 to 0.05.

Normalised distribution of the scaled momentum as a function of Q**2 in the X range 0.05 to 0.1.

Normalised distribution of the scaled momentum as a function of Q**2 in the X range 0.1 to 0.2.

Normalised distribution of the scaled momentum as a function of Q**2 in the X range 0.2 to 0.3.

Normalised distribution of the scaled momentum as a function of Q**2 in the X range 0.3 to 0.4.

Normalised distribution of the scaled momentum as a function of Q**2 in the X range 0.4 to 0.5.

Normalised distribution of the scaled momentum as a function of Q**2 in the X range 0.5 to 0.7.

Normalised distribution of the scaled momentum as a function of Q**2 in the X range 0.7 to 1.

PI+ multiplicty ratio (Helium/Deuterium) as a function of Z.

K+ multiplicty ratio (Helium/Deuterium) as a function of Z.

P multiplicty ratio (Helium/Deuterium) as a function of Z.

PI+ multiplicty ratio (Helium/Deuterium) as a function of Q**2.

K+ multiplicty ratio (Helium/Deuterium) as a function of Q**2.

P multiplicty ratio (Helium/Deuterium) as a function of Q**2.

PI+ multiplicty ratio (Neon/Deuterium) as a function of NU.

K+ multiplicty ratio (Neon/Deuterium) as a function of NU.

P multiplicty ratio (Neon/Deuterium) as a function of NU.

PI+ multiplicty ratio (Neon/Deuterium) as a function of Z.

K+ multiplicty ratio (Neon/Deuterium) as a function of Z.

P multiplicty ratio (Neon/Deuterium) as a function of Z.

PI+ multiplicty ratio (Neon/Deuterium) as a function of Q**2.

K+ multiplicty ratio (Neon/Deuterium) as a function of Q**2.

P multiplicty ratio (Neon/Deuterium) as a function of Q**2.

PI+ multiplicty ratio (Krypton/Deuterium) as a function of NU.

K+ multiplicty ratio (Krypton/Deuterium) as a function of NU.

P multiplicty ratio (Krypton/Deuterium) as a function of NU.

PI+ multiplicty ratio (Krypton/Deuterium) as a function of Z.

K+ multiplicty ratio (Krypton/Deuterium) as a function of Z.

P multiplicty ratio (Krypton/Deuterium) as a function of Z.

PI+ multiplicty ratio (Krypton/Deuterium) as a function of Q**2.

K+ multiplicty ratio (Krypton/Deuterium) as a function of Q**2.

P multiplicty ratio (Krypton/Deuterium) as a function of Q**2.

PI+ multiplicty ratio (Xenon/Deuterium) as a function of NU.

K+ multiplicty ratio (Xenon/Deuterium) as a function of NU.

P multiplicty ratio (Xenon/Deuterium) as a function of NU.

PI+ multiplicty ratio (Xenon/Deuterium) as a function of Z.

K+ multiplicty ratio (Xenon/Deuterium) as a function of Z.

P multiplicty ratio (Xenon/Deuterium) as a function of Z.

PI+ multiplicty ratio (Xenon/Deuterium) as a function of Q**2.

K+ multiplicty ratio (Xenon/Deuterium) as a function of Q**2.

P multiplicty ratio (Xenon/Deuterium) as a function of Q**2.

PI- multiplicity ratio (Helium/Deuterium) as a function of NU.

K- multiplicity ratio (Helium/Deuterium) as a function of NU.

PBAR multiplicity ratio (Helium/Deuterium) as a function of NU.

PI- multiplicity ratio (Helium/Deuterium) as a function of Z.

K- multiplicity ratio (Helium/Deuterium) as a function of Z.

PBAR multiplicity ratio (Helium/Deuterium) as a function of Z.

PI- multiplicity ratio (Helium/Deuterium) as a function of Q**2.

K- multiplicity ratio (Helium/Deuterium) as a function of Q**2.

PBAR multiplicity ratio (Helium/Deuterium) as a function of Q**2.

PI- multiplicity ratio (Neon/Deuterium) as a function of NU.

K- multiplicity ratio (Neon/Deuterium) as a function of NU.

PBAR multiplicity ratio (Neon/Deuterium) as a function of NU.

PI- multiplicity ratio (Neon/Deuterium) as a function of Z.

K- multiplicity ratio (Neon/Deuterium) as a function of Z.

PBAR multiplicity ratio (Neon/Deuterium) as a function of Z.

PI- multiplicity ratio (Neon/Deuterium) as a function of Q**2.

K- multiplicity ratio (Neon/Deuterium) as a function of Q**2.

PBAR multiplicity ratio (Neon/Deuterium) as a function of Q**2.

PI- multiplicity ratio (Krypton/Deuterium) as a function of NU.

K- multiplicity ratio (Krypton/Deuterium) as a function of NU.

PBAR multiplicity ratio (Krypton/Deuterium) as a function of NU.

PI- multiplicity ratio (Krypton/Deuterium) as a function of Z.

K- multiplicity ratio (Krypton/Deuterium) as a function of Z.

PBAR multiplicity ratio (Krypton/Deuterium) as a function of Z.

PI- multiplicity ratio (Krypton/Deuterium) as a function of Q**2.

K- multiplicity ratio (Krypton/Deuterium) as a function of Q**2.

PBAR multiplicity ratio (Krypton/Deuterium) as a function of Q**2.

PI- multiplicity ratio (Xenon/Deuterium) as a function of NU.

K- multiplicity ratio (Xenon/Deuterium) as a function of NU.

PBAR multiplicity ratio (Xenon/Deuterium) as a function of NU.

PI- multiplicity ratio (Xenon/Deuterium) as a function of Z.

K- multiplicity ratio (Xenon/Deuterium) as a function of Z.

PBAR multiplicity ratio (Xenon/Deuterium) as a function of Z.

PI- multiplicity ratio (Xenon/Deuterium) as a function of Q**2.

K- multiplicity ratio (Xenon/Deuterium) as a function of Q**2.

PBAR multiplicity ratio (Xenon/Deuterium) as a function of Q**2.

PI+ multiplicity ratio (Helium/Deuterium) as a function of PT**2.

K+ multiplicity ratio (Helium/Deuterium) as a function of PT**2.

P multiplicity ratio (Helium/Deuterium) as a function of PT**2.

PI- multiplicity ratio (Helium/Deuterium) as a function of PT**2.

K- multiplicity ratio (Helium/Deuterium) as a function of PT**2.

PBAR multiplicity ratio (Helium/Deuterium) as a function of PT**2.

PI+ multiplicity ratio (Neon/Deuterium) as a function of PT**2.

K+ multiplicity ratio (Neon/Deuterium) as a function of PT**2.

P multiplicity ratio (Neon/Deuterium) as a function of PT**2.

PI- multiplicity ratio (Neon/Deuterium) as a function of PT**2.

K- multiplicity ratio (Neon/Deuterium) as a function of PT**2.

PBAR multiplicity ratio (Neon/Deuterium) as a function of PT**2.

PI+ multiplicity ratio (Krypton/Deuterium) as a function of PT**2.

K+ multiplicity ratio (Krypton/Deuterium) as a function of PT**2.

P multiplicity ratio (Krypton/Deuterium) as a function of PT**2.

PI- multiplicity ratio (Krypton/Deuterium) as a function of PT**2.

K- multiplicity ratio (Krypton/Deuterium) as a function of PT**2.

PBAR multiplicity ratio (Krypton/Deuterium) as a function of PT**2.

PI+ multiplicity ratio (Xenon/Deuterium) as a function of PT**2.

K+ multiplicity ratio (Xenon/Deuterium) as a function of PT**2.

P multiplicity ratio (Xenon/Deuterium) as a function of PT**2.

PI- multiplicity ratio (Xenon/Deuterium) as a function of PT**2.

K- multiplicity ratio (Xenon/Deuterium) as a function of PT**2.

PBAR multiplicity ratio (Xenon/Deuterium) as a function of PT**2.

PI0 multiplicity ratio (Helium/Deuterium) as a function of NU.

PI0 multiplicity ratio (Helium/Deuterium) as a function of Z.

PI0 multiplicity ratio (Helium/Deuterium) as a function of Q**2.

PI0 multiplicity ratio (Helium/Deuterium) as a function of PT**2.

PI0 multiplicity ratio (Neon/Deuterium) as a function of NU.

PI0 multiplicity ratio (Neon/Deuterium) as a function of Z.

PI0 multiplicity ratio (Neon/Deuterium) as a function of Q**2.

PI0 multiplicity ratio (Neon/Deuterium) as a function of PT**2.

PI0 multiplicity ratio (Krypton/Deuterium) as a function of NU.

PI0 multiplicity ratio (Krypton/Deuterium) as a function of Z.

PI0 multiplicity ratio (Krypton/Deuterium) as a function of Q**2.

PI0 multiplicity ratio (Krypton/Deuterium) as a function of PT**2.

PI0 multiplicity ratio (Xenon/Deuterium) as a function of NU.

PI0 multiplicity ratio (Xenon/Deuterium) as a function of Z.

PI0 multiplicity ratio (Xenon/Deuterium) as a function of Q**2.

PI0 multiplicity ratio (Xenon/Deuterium) as a function of PT**2.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of NU for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of NU for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of NU for Z > 0.7.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of Q**2 for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of Q**2 for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of Q**2 for Z > 0.7.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of PT**2 for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of PT**2 for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of PT**2 for Z > 0.7.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of NU for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of NU for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of NU for Z > 0.7.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of Q**2 for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of Q**2 for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of Q**2 for Z > 0.7.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of PT**2 for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of PT**2 for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of PT**2 for Z > 0.7.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of NU for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of NU for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of NU for Z > 0.7.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of Q**2 for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of Q**2 for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of Q**2 for Z > 0.7.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of PT**2 for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of PT**2 for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of PT**2 for Z > 0.7.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of NU for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of NU for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of NU for Z > 0.7.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of Q**2 for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of Q**2 for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of Q**2 for Z > 0.7.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of PT**2 for Z 0.2 TO 0.4.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of PT**2 for Z 0.4 TO 0.7.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of PT**2 for Z > 0.7.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of Z for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of Z for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of Z for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of Q**2 for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of Q**2 for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of Q**2 for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of PT**2 for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of PT**2 for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Helium/Deuterium) as a function of PT**2 for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of Z for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of Z for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of Z for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of Q**2 for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of Q**2 for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of Q**2 for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of PT**2 for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of PT**2 for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Neon/Deuterium) as a function of PT**2 for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of Z for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of Z for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of Z for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of Q**2 for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of Q**2 for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of Q**2 for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of PT**2 for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of PT**2 for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Krypton/Deuterium) as a function of PT**2 for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of Z for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of Z for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of Z for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of Q**2 for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of Q**2 for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of Q**2 for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of PT**2 for NU 6 TO 12 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of PT**2 for NU 12 TO 17 GeV.

Charged pion multiplicity ratio(Xenon/Deuterium) as a function of PT**2 for NU 17 TO 23.5 GeV.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of NU for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of NU for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of Z for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of Z for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of Q**2 for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of Q**2 for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of NU for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of NU for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of Z for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of Z for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of Q**2 for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of Q**2 for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of NU for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of NU for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of Z for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of Z for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of Q**2 for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of Q**2 for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of NU for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of NU for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of Z for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of Z for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of Q**2 for PT**2 < 0.7 GeV**2.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of Q**2 for PT**2 > 0.7 GeV**2.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 20 TO 23.5 GeV.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 17 TO 20 GeV.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 14 TO 17 GeV.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 11 TO 14 GeV.

Charged pion multiplicity ratio (Helium/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 6 TO 11 GeV.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 20 TO 23.5 GeV.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 17 TO 20 GeV.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 14 TO 17 GeV.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 11 TO 14 GeV.

Charged pion multiplicity ratio (Neon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 6 TO 11 GeV.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 20 TO 23.5 GeV.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 17 TO 20 GeV.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 14 TO 17 GeV.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 11 TO 14 GeV.

Charged pion multiplicity ratio (Krypton/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 6 TO 11 GeV.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 20 TO 23.5 GeV.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 17 TO 20 GeV.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 14 TO 17 GeV.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 11 TO 14 GeV.

Charged pion multiplicity ratio (Xenon/Deuterium) as a function of the formation Length Lc (see text of paper). for NU 6 TO 11 GeV.

Differential cross section for XI- production.

Differential cross section for XI(1530)0 production.

Differential cross section for XI(1530)0 production.

Differential cross section for LAMBDA production.

Differential cross section for LAMBDA production.

Differential cross section for XI- production.

Mean number per hadronic event in the restricted PT and ETARAP phase space.

Mean number per hadronic event extrapolated to the full phase space.

K0S inclusive invariant PT distribution for HARD events at a centre of massenergy 630 GeV.

K0S inclusive invariant PT distribution for MB events at a centre of mass energy 630 GeV.

K0S inclusive invariant PT distribution for SOFT events at a centre of massenergy 630 GeV.

LAMBDA inclusive invariant PT distribution for HARD events at a centre of mass energy 1800 GeV.

LAMBDA inclusive invariant PT distribution for MB events at a centre of mass energy 1800 GeV.

LAMBDA inclusive invariant PT distribution for SOFT events at a centre of mass energy 1800 GeV.

LAMBDA inclusive invariant PT distribution for HARD events at a centre of mass energy 630 GeV.

LAMBDA inclusive invariant PT distribution for MB events at a centre of mass energy 630 GeV.

LAMBDA inclusive invariant PT distribution for SOFT events at a centre of mass energy 630 GeV.

Average PT of K0S at a centre of mass 1800 GeV for the MB data sample.

Average PT of LAMBDA at a centre of mass 1800 GeV for the MB data sample.

Average PT of K0S at a centre of mass 1800 GeV for the SOFT data sample.

Average PT of LAMBDA at a centre of mass 1800 GeV for the SOFT data sample.

Average PT of K0S at a centre of mass 1800 GeV for the HARD data sample.

Average PT of LAMBDA at a centre of mass 1800 GeV for the HARD data sample.

Average PT of K0S at a centre of mass 630 GeV for the MB data sample.

Average PT of LAMBDA at a centre of mass 630 GeV for the MB data sample.

Average PT of K0S at a centre of mass 630 GeV for the SOFT data sample.

Average PT of LAMBDA at a centre of mass 630 GeV for the SOFT data sample.

Average PT of K0S at a centre of mass 630 GeV for the HARD data sample.

Average PT of LAMBDA at a centre of mass 630 GeV for the HARD data sample.

Mean number of K0S per event divided by the charged multiplicity for the HARD data sample at centre of mass energy 1800 GeV.

Mean number of K0S per event divided by the charged multiplicity for the MBdata sample at centre of mass energy 1800 GeV.

Mean number of K0S per event divided by the charged multiplicity for the SOFT data sample at centre of mass energy 1800 GeV.

Mean number of K0S per event divided by the charged multiplicity for the HARD data sample at centre of mass energy 630 GeV.

Mean number of K0S per event divided by the charged multiplicity for the MBdata sample at centre of mass energy 630 GeV.

Mean number of K0S per event divided by the charged multiplicity for the SOFT data sample at centre of mass energy 630 GeV.

Mean number of LAMBDA per event divided by the charged multiplicity for theHARD data sample at centre of mass energy 1800 GeV.

Mean number of LAMBDA per event divided by the charged multiplicity for theMB data sample at centre of mass energy 1800 GeV.

Mean number of LAMBDA per event divided by the charged multiplicity for theSOFT data sample at centre of mass energy 1800 GeV.

Mean number of LAMBDA per event divided by the charged multiplicity for theHARD data sample at centre of mass energy 630 GeV.

Mean number of LAMBDA per event divided by the charged multiplicity for theMB data sample at centre of mass energy 630 GeV.

Mean number of LAMBDA per event divided by the charged multiplicity for theSOFT data sample at centre of mass energy 630 GeV.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 172.3 GeV.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 182.8 GeV.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 188.6 GeV.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 194.4 GeV.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 200.2 GeV.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 206.2 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 130.1 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 136.1 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 161.3 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 172.3 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 182.8 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 188.6 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 194.4 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 200.2 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 206.2 GeV.

Jet fractions using the Cambridge algorithm as a function of the jet resolution parameter YCUT at c.m. energy 202.2 GeV.

Jet fractions using the Cambridge algorithm as a function of the jet resolution parameter YCUT at c.m. energy 206.2 GeV.

Differential distributions for event thrust.

Differential distributions for event thrust.

Differential distributions for event thrust.

Differential distributions for event thrust.

Differential distributions for event thrust.

Differential distributions for the scaled heavy jet mass (RHO(C=HEAVY)).

Differential distributions for the scaled heavy jet mass (RHO(C=HEAVY)).

Differential distributions for the scaled heavy jet mass (RHO(C=HEAVY)).

Differential distributions for the scaled heavy jet mass (RHO(C=HEAVY)).

Differential distributions for the scaled heavy jet mass (RHO(C=HEAVY)).

Differential distributions for total jet broadening (BT).

Differential distributions for total jet broadening (BT).

Differential distributions for total jet broadening (BT).

Differential distributions for total jet broadening (BT).

Differential distributions for total jet broadening (BT).

Differential distributions for wide jet broadening (BW).

Differential distributions for wide jet broadening (BW).

Differential distributions for wide jet broadening (BW).

Differential distributions for wide jet broadening (BW).

Differential distributions for wide jet broadening (BW).

Differential distributions for the C-Parameter.

Differential distributions for the C-Parameter.

Differential distributions for the C-Parameter.

Differential distributions for the D-Parameter.

Differential distributions for the D-Parameter.

Differential distributions for the D-Parameter.

Differential distributions for the THRUST at c.m. energy 91.2 GeV for light quark (udsc) and b quark events.

Differential distributions for the RHO(C=HEAVY) at c.m. energy 91.2 GeV forlight quark (udsc) and b quark events.

Differential distributions for the BT at c.m. energy 91.2 GeV for light quark (udsc) and b quark events.

Differential distributions for the BW at c.m. energy 91.2 GeV for light quark (udsc) and b quark events.

Differential distributions for the C-PARAM at c.m. energy 91.2 GeV for light quark (udsc) and b quark events.

Differential distributions for the D-PARAM at c.m. energy 91.2 GeV for light quark (udsc) and b quark events.

Mean values (first moment) and dispersion (second moment) of the THRUST distribution as a function of c.m. energy.

Mean values (first moment) and dispersion (second moment) of the scaled heavy jet mass (RHO(C=HEAVY)) as a function of c.m. energy.

Mean values (first moment) and dispersion (second moment) of the total jet broadening (BT) as a function of c.m. energy.

Mean values (first moment) and dispersion (second moment) of the wide jet broadening (BW) as a function of c.m. energy.

Mean values (first moment) and dispersion (second moment) of the C-PARAM as a function of c.m. energy.

Mean values (first moment) and dispersion (second moment) of the D-PARAM as a function of c.m. energy.

Charged particle multiplicities at c.m. energy 91.2 GeV for all flavour, light quark (udsc) and bottom (b) flavour events.

Charged particle multiplicity.

Charged particle multiplicity.

Charged particle multiplicity.

First and second moment of the charged particle multiplicity distribution at c.m. energy 91.2 GeV for all flavours and for udsc an b flavours.

First and second moment of the charged particle multiplicity distribution at c.m. energy.

Distribution of LN(1/X) at c.m. energy 91.2 GeV.

Distribution of LN(1/X) at higher c.m. energies.

Distribution of LN(1/X) at higher c.m. energies.

Distribution of LN(1/X) at higher c.m. energies.