HMS Luminosity Scan
Ryan Ambrose
University of Regina
April 26, 2018
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HMS Luminosity Scan Ryan Ambrose University of Regina April 26, - - PowerPoint PPT Presentation
HMS Luminosity Scan Ryan Ambrose University of Regina April 26, 2018 1 / 8 Procedure Using the TSelector framework, I applied several cuts to the data: | 1 . 0 | < 0 . 2 2 /N < 25 . 0 E Cal,Norm > 0 . 8 |
University of Regina
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◮ |β − 1.0| < 0.2 ◮ χ2/N < 25.0 ◮ ECal,Norm > 0.8 ◮ |δ| < 8.0 ◮ |θ| < 0.080 ◮ |φ| < 0.035 ◮ |BCM17 − Current| < 0.1 ∗ Current
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◮ prescaler ◮ charge ◮ computer live time ◮ electronic live time ◮ tracking efficiency
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35 40 45 50 55 60 Current uA 0.8 0.85 0.9 0.95 1 1.05 1.1 1.15 1.2 Normalized Yield / ndf
2
χ 0.006657 / 2 Intercept ± 1 Slope 0.002863 ± 0.001481 − / ndf
2
χ 0.006657 / 2 Intercept ± 1 Slope 0.002863 ± 0.001481 −
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10 20 30 40 50 60 70 80 Current uA 0.8 0.85 0.9 0.95 1 1.05 1.1 1.15 1.2 Normalized Yield / ndf
2
χ 0.4716 / 8 Intercept ± 1 Slope 0.0006209 ± 0.0006657 / ndf
2
χ 0.4716 / 8 Intercept ± 1 Slope 0.0006209 ± 0.0006657
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10 20 30 40 50 60 70 80 Current uA 0.8 0.85 0.9 0.95 1 1.05 1.1 1.15 1.2 Normalized Yield / ndf
2
χ 0.146 / 6 Intercept ± 1 Slope 0.0006604 ± 0.001023 / ndf
2
χ 0.146 / 6 Intercept ± 1 Slope 0.0006604 ± 0.001023
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◮ Refine error bars (read from scalar information
◮ Refine calculation of charge (use scalar information) ◮ Carefully account for impact of ignoring scalar events on various
◮ Apply to SHMS scans
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