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We present STAR measurements of the azimuthal anisotropy parameter $v_2$ for pions, kaons, protons, $\Lambda$, $\bar{\Lambda}$, $\Xi+\bar{\Xi}$, and $\Omega + \bar{\Omega}$, along with $v_4$ for pions, kaons, protons, and $\Lambda + \bar{\Lambda}$ at mid-rapidity for Au+Au collisions at $\sqrt{s_{_{NN}}}=62.4$ and 200 GeV. The $v_2(p_T)$ values for all hadron species at 62.4 GeV are similar to those observed in 130 and 200 GeV collisions. For observed kinematic ranges, $v_2$ values at 62.4, 130, and 200 GeV are as little as 10%--15% larger than those in Pb+Pb collisions at $\sqrt{s_{_{NN}}}=17.3$ GeV. At intermediate transverse momentum ($p_T$ from 1.5--5 GeV/c), the 62.4 GeV $v_2(p_T)$ and $v_4(p_T)$ values are consistent with the quark-number scaling first observed at 200 GeV. A four-particle cumulant analysis is used to assess the non-flow contributions to pions and protons and some indications are found for a smaller non-flow contribution to protons than pions. Baryon $v_2$ is larger than anti-baryon $v_2$ at 62.4 and 200 GeV perhaps indicating either that the initial spatial net-baryon distribution is anisotropic, that the mechanism leading to transport of baryon number from beam- to mid-rapidity enhances $v_2$, or that anti-baryon and baryon annihilation is larger in the in-plane direction.
Minimum-bias (0–80% of the collision cross section) v2(pT ) for identified hadrons at |η| < 1 from Au+Au collisions at √sNN = 62.4 GeV. To facilitate comparisons between panels, v2 values for inclusive charged hadrons are displayed in each panel. The error bars on the data points represent statistical uncertainties. Systematic uncertainties for the identified particles are shown as shaded bands around v2 = 0.
Minimum-bias (0–80% of the collision cross section) v2(pT ) for identified hadrons at |η| < 1 from Au+Au collisions at √sNN = 62.4 GeV. To facilitate comparisons between panels, v2 values for inclusive charged hadrons are displayed in each panel. The error bars on the data points represent statistical uncertainties. Systematic uncertainties for the identified particles are shown as shaded bands around v2 = 0.
Minimum-bias (0–80% of the collision cross section) v2(pT ) for identified hadrons at |η| < 1 from Au+Au collisions at √sNN = 62.4 GeV. To facilitate comparisons between panels, v2 values for inclusive charged hadrons are displayed in each panel. The error bars on the data points represent statistical uncertainties. Systematic uncertainties for the identified particles are shown as shaded bands around v2 = 0.
Minimum-bias (0–80% of the collision cross section) v2(pT ) for identified hadrons at |η| < 1 from Au+Au collisions at √sNN = 62.4 GeV. To facilitate comparisons between panels, v2 values for inclusive charged hadrons are displayed in each panel. The error bars on the data points represent statistical uncertainties. Systematic uncertainties for the identified particles are shown as shaded bands around v2 = 0.
Minimum-bias (0–80% of the collision cross section) v2(pT ) for identified hadrons at |η| < 1 from Au+Au collisions at √sNN = 62.4 GeV. To facilitate comparisons between panels, v2 values for inclusive charged hadrons are displayed in each panel. The error bars on the data points represent statistical uncertainties. Systematic uncertainties for the identified particles are shown as shaded bands around v2 = 0.
Minimum-bias (0–80% of the collision cross section) v2(pT ) for identified hadrons at |η| < 1 from Au+Au collisions at √sNN = 62.4 GeV. To facilitate comparisons between panels, v2 values for inclusive charged hadrons are displayed in each panel. The error bars on the data points represent statistical uncertainties. Systematic uncertainties for the identified particles are shown as shaded bands around v2 = 0.
Minimum-bias (0–80% of the collision cross section) v2(pT ) for identified hadrons at |η| < 1 from Au+Au collisions at √sNN = 62.4 GeV. To facilitate comparisons between panels, v2 values for inclusive charged hadrons are displayed in each panel. The error bars on the data points represent statistical uncertainties. Systematic uncertainties for the identified particles are shown as shaded bands around v2 = 0.
Minimum-bias (0–80% of the collision cross section) v2(pT ) for identified hadrons at |η| < 1 from Au+Au collisions at √sNN = 62.4 GeV. To facilitate comparisons between panels, v2 values for inclusive charged hadrons are displayed in each panel. The error bars on the data points represent statistical uncertainties. Systematic uncertainties for the identified particles are shown as shaded bands around v2 = 0.
Minimum-bias (0–80% of the collision cross section) v2(pT ) for identified hadrons at |η| < 1 from Au+Au collisions at √sNN = 62.4 GeV. To facilitate comparisons between panels, v2 values for inclusive charged hadrons are displayed in each panel. The error bars on the data points represent statistical uncertainties. Systematic uncertainties for the identified particles are shown as shaded bands around v2 = 0.
Minimum-bias (0–80% of the collision cross section) v2(pT ) for identified hadrons at |η| < 1 from Au+Au collisions at √sNN = 62.4 GeV. To facilitate comparisons between panels, v2 values for inclusive charged hadrons are displayed in each panel. The error bars on the data points represent statistical uncertainties. Systematic uncertainties for the identified particles are shown as shaded bands around v2 = 0.
Minimum-bias (0–80% of the collision cross section) v2(pT ) for identified hadrons at |η| < 1 from Au+Au collisions at √sNN = 62.4 GeV. To facilitate comparisons between panels, v2 values for inclusive charged hadrons are displayed in each panel. The error bars on the data points represent statistical uncertainties. Systematic uncertainties for the identified particles are shown as shaded bands around v2 = 0.
Minimum-bias (0–80% of the collision cross section) v2(pT ) for identified hadrons at |η| < 1 from Au+Au collisions at √sNN = 62.4 GeV. To facilitate comparisons between panels, v2 values for inclusive charged hadrons are displayed in each panel. The error bars on the data points represent statistical uncertainties. Systematic uncertainties for the identified particles are shown as shaded bands around v2 = 0.
Minimum-bias (0–80% of the collision cross section) v2(pT ) for identified hadrons at |η| < 1 from Au+Au collisions at √sNN = 62.4 GeV. To facilitate comparisons between panels, v2 values for inclusive charged hadrons are displayed in each panel. The error bars on the data points represent statistical uncertainties. Systematic uncertainties for the identified particles are shown as shaded bands around v2 = 0.
Minimum-bias (0–80% of the collision cross section) v2(pT ) for identified hadrons at |η| < 1 from Au+Au collisions at √sNN = 62.4 GeV. To facilitate comparisons between panels, v2 values for inclusive charged hadrons are displayed in each panel. The error bars on the data points represent statistical uncertainties. Systematic uncertainties for the identified particles are shown as shaded bands around v2 = 0.
Minimum-bias (0–80% of the collision cross section) v2(pT ) for identified hadrons at |η| < 1 from Au+Au collisions at √sNN = 62.4 GeV. To facilitate comparisons between panels, v2 values for inclusive charged hadrons are displayed in each panel. The error bars on the data points represent statistical uncertainties. Systematic uncertainties for the identified particles are shown as shaded bands around v2 = 0.
Minimum-bias (0–80% of the collision cross section) v2(pT ) for identified hadrons at |η| < 1 from Au+Au collisions at √sNN = 62.4 GeV. To facilitate comparisons between panels, v2 values for inclusive charged hadrons are displayed in each panel. The error bars on the data points represent statistical uncertainties. Systematic uncertainties for the identified particles are shown as shaded bands around v2 = 0.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The unidentified charged hadron, charged pion, $K^0_S$, charged kaon, proton and Λ+Λ v2 as a function of pT for 10%–40%, 0%–10% and 40%–80% of the Au+Au interaction cross section at √sNN = 62.4 GeV. Weak-decay feed-down errors are included in the error bars on the data points while non-flow and tracking error uncertainties are plotted as bands around v2 = 0, which apply to all identified particles. The errors are asymmetric and the portion of the error band above (below) zero represents the negative (positive) error.
The ratio of Λ v2 to Λbar v2. The data are from minimum bias Au+Au collisions at √sNN = 62.4 and 200 GeV. The bands show the average values of the ratios within the indicated pT ranges.
The ratio of Λ v2 to Λbar v2. The data are from minimum bias Au+Au collisions at √sNN = 62.4 and 200 GeV. The bands show the average values of the ratios within the indicated pT ranges.
The pT integrated ratio of Λ v2 to Λbar v2 for three centrality intervals 0%–10%, 10%–40%, and 40%–80%. The data are from Au+Au collisions at √sNN = 62.4 and 200 GeV.
The pT integrated ratio of Λ v2 to Λbar v2 for three centrality intervals 0%–10%, 10%–40%, and 40%–80%. The data are from Au+Au collisions at √sNN = 62.4 and 200 GeV.
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
Identified particle v2 from minimum bias collisions at √sNN = 62.4 GeV scaled by the number of valence quarks in the hadron (nq) and plotted versus pT/nq (a) and (mT − m0)/nq (b). In each case a polynomial curve is fit to all particles except pions. The ratio of v2/nq to the fit function is shown in the bottom panels (c) and (d).
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
v2/nq scaled by the mean eccentricity of the initial overlap region versus (mT − m0)/nq for 0%–10%, 10%–40%, and 40%–80% most central Au+Au collisions at √sNN = 62.4 GeV.
Top panels - minimum bias $v_4$ for pions, charged kaons, $K^0_S$, anti-protons and Λ + Λbar at √sNN = 62.4 GeV. In the left panel the solid (dashed) line shows thevalue for $v_2^2$ for pions (kaons). Intheright panel the dashedline is $v_2^2$ for Λ + Λbar. Bottom panels - $v_4$ scaled by $v_2^2$ (points where $v_4$ and $v_2$ fluctuate around zero are not plotted). Grey bands correspond to the fit results described in the text and Table II. The systematic errors on the $v_4/v_2^2$ ratio from nonflow are included in the error bars leading to asymmetric errors.
Top panels - minimum bias $v_4$ for pions, charged kaons, $K^0_S$, anti-protons and Λ + Λbar at √sNN = 62.4 GeV. In the left panel the solid (dashed) line shows thevalue for $v_2^2$ for pions (kaons). Intheright panel the dashedline is $v_2^2$ for Λ + Λbar. Bottom panels - $v_4$ scaled by $v_2^2$ (points where $v_4$ and $v_2$ fluctuate around zero are not plotted). Grey bands correspond to the fit results described in the text and Table II. The systematic errors on the $v_4/v_2^2$ ratio from nonflow are included in the error bars leading to asymmetric errors.
Top panels - minimum bias $v_4$ for pions, charged kaons, $K^0_S$, anti-protons and Λ + Λbar at √sNN = 62.4 GeV. In the left panel the solid (dashed) line shows thevalue for $v_2^2$ for pions (kaons). Intheright panel the dashedline is $v_2^2$ for Λ + Λbar. Bottom panels - $v_4$ scaled by $v_2^2$ (points where $v_4$ and $v_2$ fluctuate around zero are not plotted). Grey bands correspond to the fit results described in the text and Table II. The systematic errors on the $v_4/v_2^2$ ratio from nonflow are included in the error bars leading to asymmetric errors.
Top panels - minimum bias $v_4$ for pions, charged kaons, $K^0_S$, anti-protons and Λ + Λbar at √sNN = 62.4 GeV. In the left panel the solid (dashed) line shows thevalue for $v_2^2$ for pions (kaons). Intheright panel the dashedline is $v_2^2$ for Λ + Λbar. Bottom panels - $v_4$ scaled by $v_2^2$ (points where $v_4$ and $v_2$ fluctuate around zero are not plotted). Grey bands correspond to the fit results described in the text and Table II. The systematic errors on the $v_4/v_2^2$ ratio from nonflow are included in the error bars leading to asymmetric errors.
Top panels - minimum bias $v_4$ for pions, charged kaons, $K^0_S$, anti-protons and Λ + Λbar at √sNN = 62.4 GeV. In the left panel the solid (dashed) line shows thevalue for $v_2^2$ for pions (kaons). Intheright panel the dashedline is $v_2^2$ for Λ + Λbar. Bottom panels - $v_4$ scaled by $v_2^2$ (points where $v_4$ and $v_2$ fluctuate around zero are not plotted). Grey bands correspond to the fit results described in the text and Table II. The systematic errors on the $v_4/v_2^2$ ratio from nonflow are included in the error bars leading to asymmetric errors.
Top panels - minimum bias $v_4$ for pions, charged kaons, $K^0_S$, anti-protons and Λ + Λbar at √sNN = 62.4 GeV. In the left panel the solid (dashed) line shows thevalue for $v_2^2$ for pions (kaons). Intheright panel the dashedline is $v_2^2$ for Λ + Λbar. Bottom panels - $v_4$ scaled by $v_2^2$ (points where $v_4$ and $v_2$ fluctuate around zero are not plotted). Grey bands correspond to the fit results described in the text and Table II. The systematic errors on the $v_4/v_2^2$ ratio from nonflow are included in the error bars leading to asymmetric errors.
Top panels - minimum bias $v_4$ for pions, charged kaons, $K^0_S$, anti-protons and Λ + Λbar at √sNN = 62.4 GeV. In the left panel the solid (dashed) line shows thevalue for $v_2^2$ for pions (kaons). Intheright panel the dashedline is $v_2^2$ for Λ + Λbar. Bottom panels - $v_4$ scaled by $v_2^2$ (points where $v_4$ and $v_2$ fluctuate around zero are not plotted). Grey bands correspond to the fit results described in the text and Table II. The systematic errors on the $v_4/v_2^2$ ratio from nonflow are included in the error bars leading to asymmetric errors.
Top panels - minimum bias $v_4$ for pions, charged kaons, $K^0_S$, anti-protons and Λ + Λbar at √sNN = 62.4 GeV. In the left panel the solid (dashed) line shows thevalue for $v_2^2$ for pions (kaons). Intheright panel the dashedline is $v_2^2$ for Λ + Λbar. Bottom panels - $v_4$ scaled by $v_2^2$ (points where $v_4$ and $v_2$ fluctuate around zero are not plotted). Grey bands correspond to the fit results described in the text and Table II. The systematic errors on the $v_4/v_2^2$ ratio from nonflow are included in the error bars leading to asymmetric errors.
Top panel - $v_2$ for pions and protons at √sNN = 62.4 and 17.3 GeV. The 62.4 GeV data are from TOF and dE/dx measurements combined. Middle and bottom panel - ratios of $v_2$ for $\pi^++\pi^-$, $K^0_S$, p+p, Λ+Λbar and at different center-of-mass energies scaled by the values at 62.4 GeV. The grey and yellow bands represent systematic uncertainties in the v2 ratios arising from non-flow effects. The grey bands (above unity) are the uncertainties for the 200 GeV/62.4 GeV data and the yellow bands (below unity) are for the 17.3 GeV/62.4 GeV data.
Top panel - $v_2$ for pions and protons at √sNN = 62.4 and 17.3 GeV. The 62.4 GeV data are from TOF and dE/dx measurements combined. Middle and bottom panel - ratios of $v_2$ for $\pi^++\pi^-$, $K^0_S$, p+p, Λ+Λbar and at different center-of-mass energies scaled by the values at 62.4 GeV. The grey and yellow bands represent systematic uncertainties in the v2 ratios arising from non-flow effects. The grey bands (above unity) are the uncertainties for the 200 GeV/62.4 GeV data and the yellow bands (below unity) are for the 17.3 GeV/62.4 GeV data.
Top panel - $v_2$ for pions and protons at √sNN = 62.4 and 17.3 GeV. The 62.4 GeV data are from TOF and dE/dx measurements combined. Middle and bottom panel - ratios of $v_2$ for $\pi^++\pi^-$, $K^0_S$, p+p, Λ+Λbar and at different center-of-mass energies scaled by the values at 62.4 GeV. The grey and yellow bands represent systematic uncertainties in the v2 ratios arising from non-flow effects. The grey bands (above unity) are the uncertainties for the 200 GeV/62.4 GeV data and the yellow bands (below unity) are for the 17.3 GeV/62.4 GeV data.
Top panel - $v_2$ for pions and protons at √sNN = 62.4 and 17.3 GeV. The 62.4 GeV data are from TOF and dE/dx measurements combined. Middle and bottom panel - ratios of $v_2$ for $\pi^++\pi^-$, $K^0_S$, p+p, Λ+Λbar and at different center-of-mass energies scaled by the values at 62.4 GeV. The grey and yellow bands represent systematic uncertainties in the v2 ratios arising from non-flow effects. The grey bands (above unity) are the uncertainties for the 200 GeV/62.4 GeV data and the yellow bands (below unity) are for the 17.3 GeV/62.4 GeV data.
Top panel - $v_2$ for pions and protons at √sNN = 62.4 and 17.3 GeV. The 62.4 GeV data are from TOF and dE/dx measurements combined. Middle and bottom panel - ratios of $v_2$ for $\pi^++\pi^-$, $K^0_S$, p+p, Λ+Λbar and at different center-of-mass energies scaled by the values at 62.4 GeV. The grey and yellow bands represent systematic uncertainties in the v2 ratios arising from non-flow effects. The grey bands (above unity) are the uncertainties for the 200 GeV/62.4 GeV data and the yellow bands (below unity) are for the 17.3 GeV/62.4 GeV data.
Top panel - $v_2$ for pions and protons at √sNN = 62.4 and 17.3 GeV. The 62.4 GeV data are from TOF and dE/dx measurements combined. Middle and bottom panel - ratios of $v_2$ for $\pi^++\pi^-$, $K^0_S$, p+p, Λ+Λbar and at different center-of-mass energies scaled by the values at 62.4 GeV. The grey and yellow bands represent systematic uncertainties in the v2 ratios arising from non-flow effects. The grey bands (above unity) are the uncertainties for the 200 GeV/62.4 GeV data and the yellow bands (below unity) are for the 17.3 GeV/62.4 GeV data.
Top panel - $v_2$ for pions and protons at √sNN = 62.4 and 17.3 GeV. The 62.4 GeV data are from TOF and dE/dx measurements combined. Middle and bottom panel - ratios of $v_2$ for $\pi^++\pi^-$, $K^0_S$, p+p, Λ+Λbar and at different center-of-mass energies scaled by the values at 62.4 GeV. The grey and yellow bands represent systematic uncertainties in the v2 ratios arising from non-flow effects. The grey bands (above unity) are the uncertainties for the 200 GeV/62.4 GeV data and the yellow bands (below unity) are for the 17.3 GeV/62.4 GeV data.
Top panel - $v_2$ for pions and protons at √sNN = 62.4 and 17.3 GeV. The 62.4 GeV data are from TOF and dE/dx measurements combined. Middle and bottom panel - ratios of $v_2$ for $\pi^++\pi^-$, $K^0_S$, p+p, Λ+Λbar and at different center-of-mass energies scaled by the values at 62.4 GeV. The grey and yellow bands represent systematic uncertainties in the v2 ratios arising from non-flow effects. The grey bands (above unity) are the uncertainties for the 200 GeV/62.4 GeV data and the yellow bands (below unity) are for the 17.3 GeV/62.4 GeV data.
A measurement of the beam-spin asymmetry in the azimuthal distribution of pions produced in semi-inclusive deep-inelastic scattering off protons is presented. The measurement was performed using the {HERMES} spectrometer with a hydrogen gas target and the longitudinally polarized 27.6 GeV positron beam of HERA. The sinusoidal amplitude of the dependence of the asymmetry on the angle $\phi$ of the hadron production plane around the virtual photon direction relative to the lepton scattering plane was measured for $\pi^+,\pi^-$ and $\pi^0$ mesons. The dependence of this amplitude on the Bjorken scaling variable and on the pion fractional energy and transverse momentum is presented. The results are compared to theoretical model calculations.
Beam SSA as a function of Z, X, hadronic PT and Q**2.
Beam SSA as a function of Z, X, hadronic PT and Q**2.
Beam SSA as a function of Z, X, hadronic PT and Q**2.
Beam SSA as a function of Z, X, hadronic PT and Q**2 corrected for the decay of exclusively produced VMs with the DSYS error due to the uncertainty in the VM subtraction.
Beam SSA as a function of Z, X, hadronic PT and Q**2 corrected for the decay of exclusively produced VMs with the DSYS error due to the uncertainty in the VM subtraction.
Beam SSA as a function of Z, X, hadronic PT and Q**2 corrected for the decay of exclusively produced VMs with the DSYS error due to the uncertainty in the VM subtraction.
Differential inclusive-jet cross sections have been measured for different jet radii in neutral current deep inelastic ep scattering for boson virtualities Q^2 > 125 GeV^2 with the ZEUS detector at HERA using an integrated luminosity of 81.7 pb^-1. Jets were identified in the Breit frame using the k_T cluster algorithm in the longitudinally inclusive mode for different values of the jet radius R. Differential cross sections are presented as functions of Q^2 and the jet transverse energy, E_T,B^jet. The dependence on R of the inclusive-jet cross section has been measured for Q^2 > 125 and 500 GeV^2 and found to be linear with R in the range studied. Next-to-leading-order QCD calculations give a good description of the measurements for 0.5 <= R <= 1. A value of alpha_s(M_Z) has been extracted from the measurements of the inclusive-jet cross-section dsigma/dQ^2 with R=1 for Q^2 > 500 GeV^2: alpha_s(M_Z) = 0.1207 +- 0.0014 (stat.) -0.0033 +0.0035 (exp.) -0.0023 +0.0022 (th.). The variation of alpha_s with E_T,B^jet is in good agreement with the running of alpha_s as predicted by QCD.
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The production of the neutral strange hadrons $K^{0}_{S}$, $\Lambda$ and $\bar{\Lambda}$ has been measured in $ep$ collisions at HERA using the ZEUS detector. Cross sections, baryon-to-meson ratios, relative yields of strange and charged light hadrons, $\Lambda$ ($\bar{\Lambda}$) asymmetry and polarization have been measured in three kinematic regions: $Q^2 > 25 \gev^2$: $5 < Q^2 < 25 \gev^2$: and in photoproduction ($Q^2 \simeq 0$). In photoproduction the presence of two hadronic jets, each with at least $5 \gev$ transverse energy, was required. The measurements agree in general with Monte Carlo models and are consistent with measurements made at $e^+ e^-$ colliders, except for an enhancement of baryon relative to meson production in photoproduction.
Differential K0S cross section in DIS events as a function of transverse momentum (lab). for Q**2 from 5 to 25 GeV**2.
Differential K0S cross section in DIS events as a function of transverse momentum (lab). for Q**2 > 25 GeV**2.
Differential K0S cross section in DIS events as a function of pseudorapidity (lab). for Q**2 from 5 to 25 GeV**2.
Differential K0S cross section in DIS events as a function of pseudorapidity (lab). for Q**2 > 25 GeV**2.
Differential K0S cross section in DIS events as a function of Bjorken X. for Q**2 from 5 to 25 GeV**2.
Differential K0S cross section in DIS events as a function of Bjorken X. for Q**2 > 25 GeV**2.
Differential K0S cross section in DIS events as a function of Q**2. for Q**2 > 5 GeV**2.
Differential LAMBDA/LAMBDABAR cross section in DIS events as a function of transverse momentum (lab). for Q**2 from 5 to 25 GeV**2.
Differential LAMBDA/LAMBDABAR cross section in DIS events as a function of transverse momentum (lab). for Q**2 > 25 GeV**2.
Differential LAMBDA/LAMBDABAR cross section in DIS events as a function of pseudorapidity (lab). for Q**2 from 5 to 25 GeV**2.
Differential LAMBDA/LAMBDABAR cross section in DIS events as a function of pseudorapidity (lab). for Q**2 > 25 GeV**2.
Differential LAMBDA/LAMBDABAR cross section in DIS eventsas a function of Bjorken X. for Q**2 from 5 to 25 GeV**2.
Differential LAMBDA/LAMBDABAR cross section in DIS eventsas a function of Bjorken X. for Q**2 > 25 GeV**2.
Differential LAMBDA/LAMBDABAR cross section in DIS events as a function of Q**2. for Q**2 > 5 GeV**2.
Differential K0S cross section in photoproduction events as a function of transverse momentum (lab).
Differential K0S cross section in photoproduction events as a function of pseudorapidity (lab).
Differential K0S cross section in photoproduction events as a function of XOBS(C=GAMMA).
Differential LAMBDA/LAMBDABAR cross section in photoproduction events as a function of transverse momentum (lab).
Differential LAMBDA/LAMBDABAR cross section in photoproduction events as a function of pseudorapidity (lab).
Differential LAMBDA/LAMBDABAR cross section in photoproduction events as a function of XOBS(C=GAMMA).
Asymmetry in LAMBDA/LAMBDABAR production in DIS events as a function of transverse momentum (lab). for Q**2 > 25 GeV**2.
Asymmetry in LAMBDA/LAMBDABAR production in DIS events as a function of pseudorapidity (lab). for Q**2 > 25 GeV**2.
Asymmetry in LAMBDA/LAMBDABAR production in DIS events as a function of Bjorken X. for Q**2 > 25 GeV**2.
Asymmetry in LAMBDA/LAMBDABAR production in DIS events as a function of Q**2. for Q**2 > 25 GeV**2.
Asymmetry in LAMBDA/LAMBDABAR production in photoproduction events as a function of transverse momentum (lab).
Asymmetry in LAMBDA/LAMBDABAR production in photoproduction events as a function of pseudorapidity (lab).
Asymmetry in LAMBDA/LAMBDABAR production in photoproduction events as a function of XOBS(C=GAMMA).
LAMBDA/K0S production ratio in DIS events as a function of transverse momentum (lab). for Q**2 from 5 to 25 GeV**2.
LAMBDA/K0S production ratio in DIS events as a function of transverse momentum (lab). for Q**2 > 25 GeV**2.
LAMBDA/K0S production ratio in DIS events as a function of pseudorapidity (lab). for Q**2 from 5 to 25 GeV**2.
LAMBDA/K0S production ratio in DIS events as a function of pseudorapidity (lab). for Q**2 > 25 GeV**2.
LAMBDA/K0S production ratio in DIS events as a function of Bjorken X. for Q**2 from 5 to 25 GeV**2.
LAMBDA/K0S production ratio in DIS events as a function of Bjorken X. for Q**2 > 25 GeV**2.
LAMBDA/K0S production ratio in DIS events as a function of Q**2. for Q**2 > 5 GeV**2.
LAMBDA/K0S production ratio in DIS events as a function of Q**2. for Bjorken X from 2.0E-5 to 3.0E-4.
LAMBDA/K0S production ratio in DIS events as a function of Q**2. for Bjorken X from 3.0E-4 to 6.0E-4.
LAMBDA/K0S production ratio in DIS events as a function of Q**2. for Bjorken X from 6.0E-4 to 1.4E-3.
LAMBDA/K0S production ratio in DIS events as a function of Q**2. for Bjorken X from 1.4E-3 to 2.0E-2.
LAMBDA/K0S production ratio in DIS events as a function of Bjorken X. for Q**2 from 5.0 to 9.5 GeV**2.
LAMBDA/K0S production ratio in DIS events as a function of Bjorken X. for Q**2 from 9.5 to 25.0 GeV**2.
LAMBDA/K0S production ratio in DIS events as a function of Bjorken X. for Q**2 from 25 to 100 GeV**2.
LAMBDA/K0S production ratio in DIS events as a function of Bjorken X. for Q**2 from 100 to 500 GeV**2.
LAMBDA/K0S production ratio in photoproduction events as a function of transverse momentum (lab).
LAMBDA/K0S production ratio in photoproduction events as a function of pseudorapidity (lab).
LAMBDA/K0S production ratio in photoproduction events as a function of XOBS(C=GAMMA).
LAMBDA/K0S production ratio in photoproduction events as a function of transverse momentum (lab). for data from the fireball-enriched sample where the highest energy jet contributes no more than 30% to the total energy.
LAMBDA/K0S production ratio in photoproduction events as a function of transverse momentum (lab). for data from the fireball-depleted sample where the highest energy jet contributes at least 30% to the total energy.
LAMBDA/K0S production ratio in photoproduction events as a function of pseudorapidity (lab). for data from the fireball-enriched sample where the highest energy jet contributes no more than 30% to the total energy.
LAMBDA/K0S production ratio in photoproduction events as a function of pseudorapidity (lab). for data from the fireball-depleted sample where the highest energy jet contributes at least 30% to the total energy.
LAMBDA/K0S production ratio in photoproduction events as a function of XOBS(C=GAMMA). for data from the fireball-enriched sample where the highest energy jet contributes no more than 30% to the total energy.
LAMBDA/K0S production ratio in photoproduction events as a function of XOBS(C=GAMMA). for data from the fireball-depleted sample where the highest energy jet contributes at least 30% to the total energy.
K0S/Charged particle production ratio in DIS events as a function of transverse momentum (lab). for Q**2 > 25 GeV**2.
K0S/Charged particle production ratio in DIS events as a function of pseudorapidity (lab). for Q**2 > 25 GeV**2.
K0S/Charged particle production ratio in photoproduction events as a function of transverse momentum (lab).
K0S/Charged particle production ratio in photoproduction events as a function of pseudorapidity (lab).
K0S/Charged particle production ratio in photoproduction events as a function of transverse momentum (lab). for data from the fireball-enriched sample where the highest energy jet contributes no more than 30% to the total energy.
K0S/Charged particle production ratio in photoproduction events as a function of transverse momentum (lab). for data from the fireball-depleted sample where the highest energy jet contributes at least 30% to the total energy.
K0S/Charged particle production ratio in photoproduction events as a function of pseudorapidity (lab). for data from the fireball-enriched sample where the highest energy jet contributes no more than 30% to the total energy.
K0S/Charged particle production ratio in photoproduction events as a function of pseudorapidity (lab). for data from the fireball-depleted sample where the highest energy jet contributes at least 30% to the total energy.
The b-bbar production cross section in 920 GeV proton-nucleus fixed target collisions is measured by observing double muonic decays of b-flavored hadrons in the kinematic region $-0.3<\xF(\mu)<0.15$. A total number of $76\pm12$ b-bbar events is obtained with a likelihood fit of the signal and background simulated events to the data. The resulting cross section is $\sigbb = 16.2 \pm 2.5_{stat} \pm 2.8_{sys} \nbpn$, or, when combined with a previous Hera-B measurement of similar precision, $\sigbb = 15.4 \pm 1.7_{stat} \pm 1.2_{sys}^{uncorr.} \pm 1.9_{sys}^{corr.} \nbpn$, which is consistent with recent NLO calculations.
BOTTOM BOTTOMBAR production cross section.
BOTTOM BOTTOMBAR production cross section combined with previous HERA-B measurement.
We present a new measurement of the $B^+$ meson differential cross section $d\sigma/d p_T$ at $\sqrt{s}=1960$ GeV. The data correspond to an integrated luminosity of 739pb$^{-1}$ collected with the upgraded CDF detector (CDF II) at the Fermilab Tevatron collider. $B^+$ candidates are reconstructed through the decay $B^+ \to J/\psi K^+$, with $J/\psi \to \mu^+ \mu^-$. The integrated cross section for producing $B^+$ mesons with $p_T \geq 6$ GeV/c and $|y| \leq 1$ is measured to be $2.78 \pm 0.24 \mu$b
The differential cross section (nb/GeV/c) for B+ mesons as a function of pT.
The The B+ production cross section.
Inclusive D* production is measured in deep-inelastic ep scattering at HERA with the H1 detector. In addition, the production of dijets in events with a D* meson is investigated. The analysis covers values of photon virtuality 2< Q^2 <=100 GeV^2 and of inelasticity 0.05<= y <= 0.7. Differential cross sections are measured as a function of Q^2 and x and of various D* meson and jet observables. Within the experimental and theoretical uncertainties all measured cross sections are found to be adequately described by next-to-leading order (NLO) QCD calculations, based on the photon-gluon fusion process and DGLAP evolution, without the need for an additional resolved component of the photon beyond what is included at NLO. A reasonable description of the data is also achieved by a prediction based on the CCFM evolution of partons involving the k_T-unintegrated gluon distribution of the proton.
Visible cross section for inclusive D*+- production.
Visible cross section for inclusive D*+- production with two jets.
Ratio of visible cross sections of inclusive D*+- production with and without the two jets.
Differential cross section for inclusive D*+- production in the visible kinematic region as a function of Q**2.
Differential cross section for inclusive D*+- production in the visible kinematic region as a function of X.
Differential cross section for inclusive D*+- production in the visible kinematic region as a function of W.
Differential cross section for inclusive D*+- production in the visible kinematic region as a function of PT.
Differential cross section for inclusive D*+- production in the visible kinematic region as a function of ETARAP.
Differential cross section for inclusive D*+- production in the visible kinematic region as a function of Z.
Double differential cross section for inclusive D*+- production in bins of Q**2 and X.
Double differential cross section for inclusive D*+- production in bins of Q**2 and X.
Double differential cross section for inclusive D*+- production in bins of Q**2 and X.
Double differential cross section for inclusive D*+- production in bins of Q**2 and X.
Double differential cross section for inclusive D*+- production in bins of Q**2 and X.
Differential cross section for inclusive D*+- production as a function of Q**2 with the constraint that the transverse momentum of the D* in the virtual photon-proton centre-of-mass frame is > 2 GeV.
Differential cross section for inclusive D*+- production as a function of X with the constraint that the transverse momentum of the D* in the virtual photon-proton centre-of-mass frame is > 2 GeV.
Differential cross section for inclusive D*+- production as a function of PT with the constraint that the transverse momentum of the D* in the virtual photon-proton centre-of-mass frame is > 2 GeV.
Differential cross section for inclusive D*+- production as a function of ETARAP with the constraint that the transverse momentum of the D* in the virtualphoton-proton centre-of-mass frame is > 2 GeV.
Differential cross section for D*+- production with dijets as a function of Q**2.
Differential cross section for D*+- production with dijets as a function of X.
Differential cross section for D*+- production with dijets as a function of ET(C=JET1).
Differential cross section for D*+- production with dijets as a function of M(C=JET2).
Double differential cross section for D*+- production with dijets in bins of Q**2 and PHI(JET1)-PHI(JET2).
Double differential cross section for D*+- production with dijets in bins of Q**2 and PHI(JET1)-PHI(JET2).
Differential cross section for D*+- production with dijets as a function of pseudorapidity of the jet containing D*.
Differential cross section for D*+- production with dijets as a function of pseudorapidity of the other jet.
Differential cross section for D*+- production with dijets as a function of the pseudorapidity difference of the two jets.
Differential cross section for D*+- production with dijets as a function of X(C=GAMMA), the observed fraction of the virtual photon momentum carried by the partons.
Double differential cross section for D*+- production with dijets in bins of Q**2 and X(C=GAMMA), the observed fraction of the virtual photon momentum carried by the partons.
Differential cross section for D*+- production with dijets as a function of X(C=GLUON), the observed fraction of the proton momentum carried by the gluon.
Double differential cross section for D*+- production with dijets in bins of Q**2 and X(C=GLUON), the observed fraction of the proton momentum carried by the gluon.
Spin transfer from circularly polarized real photons to recoiling hyperons has been measured for the reactions $\vec\gamma + p \to K^+ + \vec\Lambda$ and $\vec\gamma + p \to K^+ + \vec\Sigma^0$. The data were obtained using the CLAS detector at Jefferson Lab for center-of-mass energies $W$ between 1.6 and 2.53 GeV, and for $-0.85<\cos\theta_{K^+}^{c.m.}< +0.95$. For the $\Lambda$, the polarization transfer coefficient along the photon momentum axis, $C_z$, was found to be near unity for a wide range of energy and kaon production angles. The associated transverse polarization coefficient, $C_x$, is smaller than $C_z$ by a roughly constant difference of unity. Most significantly, the {\it total} $\Lambda$ polarization vector, including the induced polarization $P$, has magnitude consistent with unity at all measured energies and production angles when the beam is fully polarized. For the $\Sigma^0$ this simple phenomenology does not hold. All existing hadrodynamic models are in poor agreement with these results.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 1.032 GeV and W = 1.679 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 1.132 GeV and W = 1.734 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 1.232 GeV and W = 1.787 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 1.332 GeV and W = 1.839 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 1.433 GeV and W = 1.889 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 1.534 GeV and W = 1.939 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 1.635 GeV and W = 1.987 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 1.737 GeV and W = 2.035 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 1.838 GeV and W = 2.081 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 1.939 GeV and W = 2.126 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 2.039 GeV and W = 2.170 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 2.139 GeV and W = 2.212 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 2.240 GeV and W = 2.255 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 2.341 GeV and W = 2.296 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 2.443 GeV and W = 2.338 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 2.543 GeV and W = 2.377 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 2.642 GeV and W = 2.416 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ LAMBDA for incident energy = 2.741 GeV and W = 2.454 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ SIGMA0 for incident energy = 1.232 GeV and W = 1.787 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ SIGMA0 for incident energy = 1.332 GeV and W = 1.839 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ SIGMA0 for incident energy = 1.433 GeV and W = 1.889 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ SIGMA0 for incident energy = 1.534 GeV and W = 1.939 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ SIGMA0 for incident energy = 1.635 GeV and W = 1.987 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ SIGMA0 for incident energy = 1.737 GeV and W = 2.035 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ SIGMA0 for incident energy = 1.838 GeV and W = 2.081 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ SIGMA0 for incident energy = 1.939 GeV and W = 2.126 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ SIGMA0 for incident energy = 2.039 GeV and W = 2.170 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ SIGMA0 for incident energy = 2.139 GeV and W = 2.212 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ SIGMA0 for incident energy = 2.240 GeV and W = 2.255 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ SIGMA0 for incident energy = 2.341 GeV and W = 2.296 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ SIGMA0 for incident energy = 2.443 GeV and W = 2.338 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ SIGMA0 for incident energy = 2.543 GeV and W = 2.377 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ SIGMA0 for incident energy = 2.642 GeV and W = 2.416 GeV.
Coefficients Cx and Cz for the reaction GAMMA P --> K+ SIGMA0 for incident energy = 2.741 GeV and W = 2.454 GeV.
Measurements of the analysing power for the p(pol)p --> ppeta reaction have been performed in the close-to-threshold energy region at beam momenta of p_{beam}=2.010 and 2.085 GeV/c, corresponding to excess energies of Q=10 and 36 MeV, respectively. The determined analysing power is essentially consistent with zero implying that the eta meson is produced predominantly in the s-wave at both excess energies. The angular dependence of the analysing power, combined with the hitherto determined isospin dependence of the total cross section for the eta meson production in nucleon-nucleon collisions, reveal a statistically significant indication that the excitation of the nucleon to the S_{11}(1535) resonance, the process which intermediates the production of the eta meson, is predominantly due to the exchange of the pi meson between the colliding nucleons.
Analysing power measurements for excess energy 10 MeV.
Analysing power measurements for excess energy 36 MeV.
We report measurements of the exclusive electroproduction of $K^+\Lambda$ and $K^+\Sigma^0$ final states from a proton target using the CLAS detector at the Thomas Jefferson National Accelerator Facility. The separated structure functions $\sigma_T$, $\sigma_L$, $\sigma_{TT}$, and $\sigma_{LT}$ were extracted from the $\Phi$- and $\epsilon$-dependent differential cross sections taken with electron beam energies of 2.567, 4.056, and 4.247 GeV. This analysis represents the first $\sigma_L/\sigma_T$ separation with the CLAS detector, and the first measurement of the kaon electroproduction structure functions away from parallel kinematics. The data span a broad range of momentum transfers from $0.5\leq Q^2\leq 2.8$ GeV$^2$ and invariant energy from $1.6\leq W\leq 2.4$ GeV, while spanning nearly the full center-of-mass angular range of the kaon. The separated structure functions reveal clear differences between the production dynamics for the $\Lambda$ and $\Sigma^0$ hyperons. These results provide an unprecedented data sample with which to constrain current and future models for the associated production of strangeness, which will allow for a better understanding of the underlying resonant and non-resonant contributions to hyperon production.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.6 to 1.7 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.7 to 1.8 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.8 to 1.9 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.9 to 2.0 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.0 to 2.1 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.1 to 2.2 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.2 to 2.3 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.3 to 2.4 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.6 to 1.7 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.7 to 1.8 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.8 to 1.9 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.9 to 2.0 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.0 to 2.1 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.1 to 2.2 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.2 to 2.3 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.3 to 2.4 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.6 to 1.7 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.7 to 1.8 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.8 to 1.9 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.9 to 2.0 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.0 to 2.1 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.1 to 2.2 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.7 to 1.8 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.8 to 1.9 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.9 to 2.0 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.0 to 2.1 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.1 to 2.2 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.2 to 2.3 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.3 to 2.4 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.7 to 1.8 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.8 to 1.9 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.9 to 2.0 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.0 to 2.1 GeV.
Cross sections for incident energy 4 GeV for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.1 to 2.2 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV.
Cross sections for incident energy 2.567 GeV for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.
Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV extracted using the simultaneous EPSILON-PHI fit method.
Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV extracted using the simultaneous EPSILON-PHI fit method.
Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV extracted using the simultaneous EPSILON-PHI fit method.
Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV extracted using the simultaneous EPSILON-PHI fit method.
Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV extracted using the Rosenbluth separation technique fit method.. E98M29 E98M30 E98M31.
Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV extracted using the Rosenbluth separation technique fit method.. E98M29 E98M30 E98M31.
Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV extracted using the Rosenbluth separation technique fit method.. E98M29 E98M30 E98M31.
Cross sections for the K+ LAMBDA data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV extracted using the Rosenbluth separation technique fit method.. E98M29 E98M30 E98M31.
Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV extracted using the simultaneous EPSILON-PHI fit method.
Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV extracted using the simultaneous EPSILON-PHI fit method.
Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV extracted using the simultaneous EPSILON-PHI fit method.
Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV extracted using the Rosenbluth separation technique fit method.. E99M29 E99M30 E99M31.
Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV extracted using the Rosenbluth separation technique fit method.. E99M29 E99M30 E99M31.
Cross sections for the K+ SIGMA0 data for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV extracted using the Rosenbluth separation technique fit method.. E99M29 E99M30 E99M31.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.
Differential cross ssection as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.70 to 1.75 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.75 to 1.80 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.80 to 1.85 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.85 to 1.90 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.90 to 1.95 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.95 to 2.00 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeVand the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeVand the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeVand the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeVand the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeVand the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeVand the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeVand the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeVand the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeVand the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeVand the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeVand the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.70 to 1.75 GeVand the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeVand the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeVand the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeVand the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeVand the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeVand the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.75 to 1.80 GeVand the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeVand the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeVand the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeVand the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeVand the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeVand the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.80 to 1.85 GeVand the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeVand the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeVand the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeVand the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeVand the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeVand the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.85 to 1.90 GeVand the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeVand the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeVand the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeVand the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeVand the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeVand the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.90 to 1.95 GeVand the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeVand the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeVand the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeVand the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeVand the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeVand the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.95 to 2.00 GeVand the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeVand the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeVand the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeVand the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeVand the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeVand the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.5 to 0.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) range 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.8 to -0.4.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.4 to -0.1.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.2 to 0.5.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) range 0.5 to 0.8.
Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.9 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges -0.8 to -0.4,. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges 0.2 to 0.5,. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 0.8 to 1.3 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges -0.8 to -0.4. -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.3 to 1.8 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges 0.2 to 0.5. 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 1.8 to 2.3 GeV**2 and W range 2.3 to 2.4 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.6 to 1.7 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.7 to 1.8 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.8 to 1.9 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 1.9 to 2.0 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.0 to 2.1 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.1 to 2.2 GeV and the COS(THETA) ranges 0.2 to 0.5, 0.5 to 0.8 and 0.8 to 1.0.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges -0.8 to -0.4, -0.4 to -0.1 and -0.1 to 0.2.
Differential cross section as a function of PHI for the Q**2 range 2.3 to 2.8 GeV**2 and W range 2.2 to 2.3 GeV and the COS(THETA) ranges 0.2 to 0.5, and.
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