<html>
  <head>

    <meta http-equiv="content-type" content="text/html; charset=utf-8">
  </head>
  <body text="#000000" bgcolor="#FFFFFF">
    Folks,<br>
    <br>
    Find the minutes below and at <a class="moz-txt-link-freetext" href="https://goo.gl/oSkcUo">https://goo.gl/oSkcUo</a> .<br>
    <br>
      -- Mark<br>
    _____________________<br>
    <div id="globalWrapper">
      <div id="column-content">
        <div id="content" class="mw-body" role="main">
          <h1 id="firstHeading" class="firstHeading" lang="en"><span
              dir="auto">GlueX Start Counter Meeting, June 30, 2016, </span><span
              class="mw-headline" id="Minutes">Minutes</span></h1>
          <div id="bodyContent" class="mw-body-content">
            <div id="mw-content-text" dir="ltr" class="mw-content-ltr"
              lang="en">
              <p>Present:
              </p>
              <ul>
                <li> <b>FIU</b>: Mahmoud Kamel</li>
                <li> <b>JLab</b>: Mark Ito (chair), Simon Taylor, Beni
                  Zihlmann</li>
                <li> <b>NU</b>: Sean Dobbs</li>
              </ul>
              <h3><span class="mw-headline" id="Update_on_Efficiencies">Update
                  on Efficiencies</span></h3>
              <p>Mahmoud presented <a rel="nofollow" class="external
                  text"
                  href="https://halldweb.jlab.org/talks/2016/ST_meeting_June30_2016.pdf">slides
                  on the latest results</a> from his efficiency studies.
                He used a ROOT tree produced from the start counter
                efficiency plugin run as part of the production
                reconstruction pass on the Spring 2016 data. A single
                file was analyzed. See his slides for the plots. His
                slides covered:
              </p>
              <ul>
                <li> criteria for selection of charged tracks in the
                  study</li>
                <li> histograms of some global properties of the tracks
                  and start counter hits</li>
                <li> start counter efficiencies for all tracks: 98%</li>
                <li> histograms of the same global properties when a phi
                  cut is applied to tracks to keep them away from the
                  edges of the counters (delta phi cut)</li>
                <li> efficiencies with the delta phi cut: 99%</li>
                <li> same efficiencies for the straight section: 99%</li>
                <li> for the bend section: 99%</li>
                <li> and for the nose section: 99%</li>
                <li> the studies were repeated for protons, pi+, pi-,
                  and K+</li>
                <li> for K+ no start counter misses were found when the
                  delta phi cut was applied; the study was repeated
                  without the cut</li>
              </ul>
              <p>Efficiencies are everywhere (almost incredibly) high.
              </p>
              <h3><span class="mw-headline" id="Calibration">Calibration</span></h3>
              <p>We asked Mahmoud to think about documenting the
                calibration procedure in a cookbook-like fashion so that
                future students will be able to reproduce it.
              </p>
              <h3><span class="mw-headline" id="Dark_Rate_Monitoring">Dark
                  Rate Monitoring</span></h3>
              <p>Beni brought us the issue of monitoring dark rate of
                the SiPMs. We don't have a regular procedure for doing
                so. This is important given the start counter's
                proximity to the beamline and Yi Qiang's study that
                degradation can occur with exposure to the beam. We will
                have to develop a way to keep track of this.
              </p>
              <h3><span class="mw-headline" id="Mcsmear_Parameters">Mcsmear
                  Parameters</span></h3>
              <p>Sean reminded Mark and Simon that they promised to come
                up with a sensible parametrization for the smearing
                function.
              </p>
              <p>He also mentioned that there is no run-dependent time
                resolution currently in the CCDB. Mahmoud has seen
                evidence for small shifts, but has not done a detailed
                time-dependence study. He will have a look, hopefully
                before the end of July.
              </p>
            </div>
            <div class="printfooter">
              Retrieved from "<a dir="ltr"
href="https://halldweb.jlab.org/wiki/index.php?title=GlueX_Start_Counter_Meeting,_June_30,_2016&oldid=75962">https://halldweb.jlab.org/wiki/index.php?title=GlueX_Start_Counter_Meeting,_June_30,_2016&oldid=75962</a>"</div>
          </div>
        </div>
      </div>
      <div id="footer" role="contentinfo">
        <ul id="f-list">
          <li id="lastmod"> This page was last modified on 30 June 2016,
            at 13:53.</li>
        </ul>
      </div>
    </div>
    <br>
    <pre class="moz-signature" cols="72">-- 
<a class="moz-txt-link-abbreviated" href="mailto:marki@jlab.org">marki@jlab.org</a>, (757)269-5295
</pre>
  </body>
</html>