<div dir="ltr">Dear Marco,<div><br></div><div>As we discussed at the today's meeting, attached is our inclusive study summary including GEMC simulations with Micromegas. It also has a comparison between CLAS12 and CLAS6.</div><div><br></div><div>10 GeV data: New (5.6.1 version), OLD (5b.3.10)</div><div>6 GeV data: OLD (5b.3.10) only</div><div>2 GeV data: OLD (5b.3.10) only</div><div><br></div><div>As soon as we have new cooking data for 2 GeV and 6 GeV available, we will include them, but I don't expect to see substantial difference since we don't see from 10 GeV. </div><div><br></div><div>The following is the summary of the file.</div><div><br></div><div>Page 1: Comparison bgetween OLD and NEW in W and Q2 vs. W. </div><div> I don't see much difference between the two.</div><div><br></div><div>Page 2: Q2 vs W spectrum. </div><div> Left Column: 2 GeV Middle column: 6 GeV Right Column: 10 GeV</div><div> Top row: CLAS12 data Middle row: GEMC simulations Bottom row: CLAS6 data from e1e and e1f</div><div><br></div><div>Page 3: W spectrum comparison between CLAS12 data and GEMC simulations</div><div> </div><div>Page 4: CLAS12 data and GEMC simulations for each sector for 2 GeV</div><div><br></div><div>Page 5:
<span style="font-size:small;background-color:rgb(255,255,255);text-decoration-style:initial;text-decoration-color:initial;float:none;display:inline"><span> </span>CLAS12 data and GEMC simulations for each sector for 6 GeV</span>
</div><div><span style="font-size:small;background-color:rgb(255,255,255);text-decoration-style:initial;text-decoration-color:initial;float:none;display:inline"><br></span></div><div><span style="font-size:small;background-color:rgb(255,255,255);text-decoration-style:initial;text-decoration-color:initial;float:none;display:inline">
<div style="text-decoration-style:initial;text-decoration-color:initial">Page 6: <span> </span><span style="font-size:small;background-color:rgb(255,255,255);text-decoration-style:initial;text-decoration-color:initial;float:none;display:inline"><span> </span>CLAS12 data and GEMC simulations for each sector for 10 GeV</span></div><div style="text-decoration-style:initial;text-decoration-color:initial"><span style="font-size:small;background-color:rgb(255,255,255);text-decoration-style:initial;text-decoration-color:initial;float:none;display:inline"><br></span></div><br class="m_4348821643027696613gmail-Apple-interchange-newline">
<br></span></div><div><br></div><div><br></div><div class="gmail_extra"><br><div class="gmail_quote">On Wed, Aug 8, 2018 at 1:30 PM, Marco Contalbrigo <span dir="ltr"><<a href="mailto:mcontalb@fe.infn.it" target="_blank">mcontalb@fe.infn.it</a>></span> wrote:<br><blockquote class="gmail_quote" style="margin:0 0 0 .8ex;border-left:1px #ccc solid;padding-left:1ex">Dear all,<br>
let me remind there will be a DPANA meeting tomorrow,<br>
Thursday 9th at 8:30 am EST.<br>
<br>
Stefan, Giovanni, Pierre and Aram will report their<br>
initial findings on the new 5.6.1 produced data. As<br>
usual, everybody is welcome to contribute with<br>
his/her study.<span><br>
<br>
Hope to see you at the meeting. Below the coordinates.<br>
<br></span><span>
JLab seminar room: F226<br>
<br>
Agenda of the meeting available at:<br>
<a href="https://clas12-docdb.jlab.org/cgi-bin/DocDB/private/DisplayMeeting?conferenceid=9" rel="noreferrer" target="_blank">https://clas12-docdb.jlab.org/<wbr>cgi-bin/DocDB/private/DisplayM<wbr>eeting?conferenceid=9</a><br>
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<br>
On Thu, 2 Aug 2018, Marco Contalbrigo wrote:<br>
<br>
</span><blockquote class="gmail_quote" style="margin:0 0 0 .8ex;border-left:1px #ccc solid;padding-left:1ex"><span>
Dear all,<br>
the deep-process meeting will be next week, on Thursday August<br>
9th morning at 8:30 EST.<br>
<br>
The meeting will focus on the analysis of the latest produced<br>
runs. The software release is tagged 5.6.1 and data is available<br>
both in full hipo files and (for a subsample) in dst formats at:<br>
<br>
/work/clas12/clas12/data/calib<wbr>/cooked_5bp6p1/<br>
/work/clas12/clas12/data/calib<wbr>/dst_5bp6p1/<br>
<br>
It would be important that analyzers run their codes on these<br>
data and provide at the meeting their feedbacks on data<br>
quality, statistics and output formats for a prompt<br>
evaluation of the present reconstruction stream.<br>
<br>
See you at the meeting, Marco.<br>
<br>
</span><blockquote class="gmail_quote" style="margin:0 0 0 .8ex;border-left:1px #ccc solid;padding-left:1ex"><blockquote class="gmail_quote" style="margin:0 0 0 .8ex;border-left:1px #ccc solid;padding-left:1ex">
<br>
<blockquote class="gmail_quote" style="margin:0 0 0 .8ex;border-left:1px #ccc solid;padding-left:1ex"><span>
JLab seminar room: F226<br>
<br>
Agenda of the meeting available at:<br>
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</span></blockquote>
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</blockquote>
<br>
</blockquote>
<br>
</blockquote><div class="m_4348821643027696613HOEnZb"><div class="m_4348821643027696613h5">
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</div></div></blockquote></div><br><br clear="all"><div><br></div>-- <br><div class="m_4348821643027696613gmail_signature" data-smartmail="gmail_signature"><div>Kyungseon Joo</div><div>Professor of Physics</div><div>University of Connecticut</div><div>Storrs, CT 06269</div><div><a href="https://urldefense.proofpoint.com/v2/url?u=http-3A__www.phys.uconn.edu_-7Ekjoo&d=DwMFaQ&c=lz9TcOasaINaaC3U7FbMev2lsutwpI4--09aP8Lu18s&r=VX70eZFUAkN25MzbimADcwXq-GV00MydhomdtiZFTu0&m=liRtQcHL0dOLx7oHK6_XNLVaMYQJ_ADwyPsvIKyo4cI&s=qfLnC_UjoUkameJbjhaCZQk3CISn_82vQcTuO9sWjqg&e=" target="_blank">http://www.phys.uconn.edu/~<wbr>kjoo</a></div></div>
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