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Dear Ken
<div>It would be great if you could do some fitting</div>
<div>And we have also 6.5GeV</div>
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<div>Best regards</div>
<div>Latifa</div>
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<div id="AppleMailSignature" dir="ltr">Sent from my iPhone</div>
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On Jun 20, 2019, at 12:04 PM, Hicks, Kenneth <<a href="mailto:hicks@ohio.edu">hicks@ohio.edu</a>> wrote:<br>
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<p class="MsoNormal"><span style="font-family:Calibri;color:black">Dear rgk people,<o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-family:Calibri;color:black"><o:p> </o:p></span></p>
<p class="MsoNormal"><span style="font-family:Calibri;color:black">Attached are two plots, one showing the W distribution for the events in the skim8_ep train for a file from the old (v2) and new (v7) cooking. It’s not the same file in both cases (run 5886
for v2, and run 5893 for v7) but these data were taken under the same conditions. I also plotted the missing mass for final state e’p’pi+ pi-.<o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-family:Calibri;color:black"><o:p> </o:p></span></p>
<p class="MsoNormal"><span style="font-family:Calibri;color:black">What I see from these plots is improved resolution. It’s hard to tell from just one file, but it appears that the new cooking has better resolution.<o:p></o:p></span></p>
<p class="MsoNormal"><span style="font-family:Calibri;color:black"><o:p> </o:p></span></p>
<p class="MsoNormal"><span style="font-family:Calibri;color:black">Best regards,<br>
ken<o:p></o:p></span></p>
<p class="MsoNormal"><span style="color:black"><o:p> </o:p></span></p>
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<div dir="ltr"><rgk-skim8-r5886-WQ2.pdf></div>
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<div dir="ltr"><rgk-skim8-r5893-WQ2.pdf></div>
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<div dir="ltr"><span>_______________________________________________</span><br>
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