<html><head><meta http-equiv="Content-Type" content="text/html charset=us-ascii"></head><body style="word-wrap: break-word; -webkit-nbsp-mode: space; -webkit-line-break: after-white-space; ">Good evening,<div><br></div><div>Karl, you're not the only one who's been nerding it up this weekend. I mean, really, who wouldn't want to spend Friday night and all day Saturday working on rates estimates? Anyway, on to your questions.</div><div><br></div><div>1) I'll move the W>2 line to W>1.8. Unless you think it makes sense to just remove it?</div><div>2) The red line on Theta_e' indicates the lowest central angle for the HMS (12.2 degrees) and the blue for the SHMS (7.3 degrees). The red line on E' indicates the maximum central momentum setting for the HMS (7.3 GeV) and the blue for the SHMS (10.4 GeV). These (and any other lines) can be easily removed if they're too confusing.</div><div>3) Give me a couple minutes and I'll send them to you</div><div>4) See below (I've split it into two tables, one with the spectrometer settings and one with our rebinned x values and what we expect for dAzz and db1):</div><div><br></div><div><div style="margin: 0px; font-size: 12px; font-family: Monaco; "><div style="margin: 0px; ">\begin{table}</div><div style="margin: 0px; ">\begin{center}</div><div style="margin: 0px; ">\begin{tabular}{c|c|c|c|cc|c|c}</div><div style="margin: 0px; ">& $\overline{x}$ & $\overline{Q^2}$ & $\overline{W}$ <span class="Apple-tab-span" style="white-space: pre; "> </span>& $P_0$ & $\theta$ & Rates & time \\</div><div style="margin: 0px; ">& ~ <span class="Apple-tab-span" style="white-space: pre; "> </span> & (GeV$^2$) <span class="Apple-tab-span" style="white-space: pre; "> </span>& (GeV) <span class="Apple-tab-span" style="white-space: pre; "> </span>& (GeV) & (deg.) & (kHz) & (days) \\</div><div style="margin: 0px; ">%\multicolumn{2}{|c|}{$\times 10^{-2}$}</div><div style="margin: 0px; ">\hline\hline</div><div style="margin: 0px; ">%Spec x Q2<span class="Apple-tab-span" style="white-space: pre; "> </span>W<span class="Apple-tab-span" style="white-space: pre; "> </span>P0<span class="Apple-tab-span" style="white-space: pre; "> </span> Theta<span class="Apple-tab-span" style="white-space: pre; "> </span> Rates<span class="Apple-tab-span" style="white-space: pre; "> </span>Time</div><div style="margin: 0px; ">SHMS & 0.15<span class="Apple-tab-span" style="white-space: pre; "> </span>& 1.21<span class="Apple-tab-span" style="white-space: pre; "> </span>& 2.78<span class="Apple-tab-span" style="white-space: pre; "> </span>& 6.70<span class="Apple-tab-span" style="white-space: pre; "> </span>& 7.35<span class="Apple-tab-span" style="white-space: pre; "> </span>& 1.66<span class="Apple-tab-span" style="white-space: pre; "> </span>& 6 \\</div><div style="margin: 0px; ">SHMS & 0.30<span class="Apple-tab-span" style="white-space: pre; "> </span>& 2.00<span class="Apple-tab-span" style="white-space: pre; "> </span>& 2.36<span class="Apple-tab-span" style="white-space: pre; "> </span>& 7.45<span class="Apple-tab-span" style="white-space: pre; "> </span>& 8.96<span class="Apple-tab-span" style="white-space: pre; "> </span>& 0.79<span class="Apple-tab-span" style="white-space: pre; "> </span>& 9 \\</div><div style="margin: 0px; ">SHMS & 0.452<span class="Apple-tab-span" style="white-space: pre; "> </span>& 2.58<span class="Apple-tab-span" style="white-space: pre; "> </span>& 2.00<span class="Apple-tab-span" style="white-space: pre; "> </span>& 7.96<span class="Apple-tab-span" style="white-space: pre; "> </span>& 9.85<span class="Apple-tab-span" style="white-space: pre; "> </span>& 0.38<span class="Apple-tab-span" style="white-space: pre; "> </span>& 15 \\</div><div style="margin: 0px; ">HMS & 0.55<span class="Apple-tab-span" style="white-space: pre; "> </span>& 3.81<span class="Apple-tab-span" style="white-space: pre; "> </span>& 2.00<span class="Apple-tab-span" style="white-space: pre; "> </span>& 7.31<span class="Apple-tab-span" style="white-space: pre; "> </span>& 12.50<span class="Apple-tab-span" style="white-space: pre; "> </span>& 0.11<span class="Apple-tab-span" style="white-space: pre; "> </span>& 30 \\ </div><div style="margin: 0px; ">\hline\hline</div><div style="margin: 0px; ">\end{tabular}</div><div style="margin: 0px; ">\caption{\label{RATES}Summary of the kinematics and physics rates using Hall C spectrometers.}</div><div style="margin: 0px; ">\end{center}</div><div style="margin: 0px; ">\end{table}</div><div><br></div></div></div><div><br></div><div><div style="margin: 0px; font-size: 12px; font-family: Monaco; ">\begin{table}</div><div style="margin: 0px; font-size: 12px; font-family: Monaco; ">\begin{center}</div><div style="margin: 0px; font-size: 12px; font-family: Monaco; ">\begin{tabular}{c|c|c|cc|cc}</div><div style="margin: 0px; font-size: 12px; font-family: Monaco; "> $\overline{x}$ & $\overline{Q^2}$ & $\overline{W}$ & $A_{zz}$ & $\delta A_{zz}^{stat}$ & $b_1$ & $\delta b_1^{stat}$ \\</div><div style="margin: 0px; font-size: 12px; font-family: Monaco; "> & (GeV$^2$) & (GeV) & \multicolumn{2}{c|}{$\times 10^{-2}$} & \multicolumn{2}{c}{$\times 10^{-2}$} \\</div><div style="margin: 0px; font-size: 12px; font-family: Monaco; ">%\multicolumn{2}{|c|}{$\times 10^{-2}$}</div><div style="margin: 0px; font-size: 12px; font-family: Monaco; ">\hline\hline</div><div style="margin: 0px; font-size: 12px; font-family: Monaco; ">% x <span class="Apple-tab-span" style="white-space: pre; "> </span> Q2<span class="Apple-tab-span" style="white-space: pre; "> </span>W<span class="Apple-tab-span" style="white-space: pre; "> </span> Azz<span class="Apple-tab-span" style="white-space: pre; "> </span> <span class="Apple-tab-span" style="white-space: pre; "> </span>dAzz <span class="Apple-tab-span" style="white-space: pre; "> </span> b1<span class="Apple-tab-span" style="white-space: pre; "> </span>db1<span class="Apple-tab-span" style="white-space: pre; "> </span></div><div style="margin: 0px; font-size: 12px; font-family: Monaco; "> 0.16<span class="Apple-tab-span" style="white-space: pre; "> </span>& 1.17<span class="Apple-tab-span" style="white-space: pre; "> </span>& 2.65 & -0.44<span class="Apple-tab-span" style="white-space: pre; "> </span>& 0.15<span class="Apple-tab-span" style="white-space: pre; "> </span>& 0.58<span class="Apple-tab-span" style="white-space: pre; "> </span>& 0.18 \\</div><div style="margin: 0px; font-size: 12px; font-family: Monaco; "> 0.28<span class="Apple-tab-span" style="white-space: pre; "> </span>& 1.76<span class="Apple-tab-span" style="white-space: pre; "> </span>& 2.35 & 0.34<span class="Apple-tab-span" style="white-space: pre; "> </span>& 0.39<span class="Apple-tab-span" style="white-space: pre; "> </span>& -0.25<span class="Apple-tab-span" style="white-space: pre; "> </span>& 0.28 \\</div><div style="margin: 0px; font-size: 12px; font-family: Monaco; "> 0.36<span class="Apple-tab-span" style="white-space: pre; "> </span>& 2.12<span class="Apple-tab-span" style="white-space: pre; "> </span>& 2.16 & 0.79<span class="Apple-tab-span" style="white-space: pre; "> </span>& 0.50<span class="Apple-tab-span" style="white-space: pre; "> </span>& -0.38<span class="Apple-tab-span" style="white-space: pre; "> </span>& 0.23 \\</div><div style="margin: 0px; font-size: 12px; font-family: Monaco; "> 0.49<span class="Apple-tab-span" style="white-space: pre; "> </span>& 3.25<span class="Apple-tab-span" style="white-space: pre; "> </span>& 2.07 & 1.35<span class="Apple-tab-span" style="white-space: pre; "> </span>& 0.37<span class="Apple-tab-span" style="white-space: pre; "> </span>& -0.27<span class="Apple-tab-span" style="white-space: pre; "> </span>& 0.08 \\ </div><div style="margin: 0px; font-size: 12px; font-family: Monaco; ">\hline\hline</div><div style="margin: 0px; font-size: 12px; font-family: Monaco; ">\end{tabular}</div><div style="margin: 0px; font-size: 12px; font-family: Monaco; ">\caption{\label{RATES}Summary of the kinematics and physics rates using Hall C spectrometers.}</div><div style="margin: 0px; font-size: 12px; font-family: Monaco; ">\end{center}</div><div style="margin: 0px; font-size: 12px; font-family: Monaco; ">\end{table}</div></div><div><br></div><div><br></div><div><br></div><div><br></div><div><br></div><div><br><div><div>On May 4, 2013, at 5:34 PM, Karl Slifer <<a href="mailto:karl.slifer@unh.edu">karl.slifer@unh.edu</a>> wrote:</div><br class="Apple-interchange-newline"><blockquote type="cite"><div dir="ltr"><br><div>Hi Ellie,</div><div><br></div><div>great, I know that probably was not very easy to put together quickly.</div><div><br></div><div>Few questions:</div><div><br></div><div>-If your assuming W>1.8, I'd move the line in the figure</div><div>-Can you explain what the horizontal lines are in the kin plots?</div><div>-Can you please provide a link to the individual plots for inclusion in the document? </div><div>-Also can you point me to the exact values I should put in Table 1 (summary of kinematics)<br></div><div><br></div><div><br></div><div>-Karl</div><div><br></div><div><br></div><div><br></div><div><br></div></div><div class="gmail_extra"><br clear="all"><div>---<br><div>Karl J. Slifer<div>Assistant Professor</div><div>University of New Hampshire<br><div>Telephone : <a>603-722-0695</a></div></div></div></div><br><br><div class="gmail_quote">On Sat, May 4, 2013 at 5:23 PM, Elena Long <<a href="mailto:ellie@jlab.org">ellie@jlab.org</a>> wrote:<br><blockquote class="gmail_quote"><div><div>Good afternoon,</div><div><br></div><div>As per Oscar's request, I've rebinned the statistical uncertainties into specific x bins. The two highest points contain data from both the SHMS and the HMS. The bins are:</div><div><br></div><div>0.09 < 0.16 < 0.23 <br>0.23 < 0.275 < 0.32 <br>0.32 < 0.36 < 0.40 </div><div>0.40 < 0.49 < 0.58 </div><div><br></div><div>I've also changed the coloring on dAzz and db1 to black so that they're not confused with the spectrometer acceptance cuts I've been showing previously, and so the PAC doesn't get confused by the colors being similar. </div><div><br></div><div>The most up-to-date plot including this can be found here: <a href="https://hallcweb.jlab.org/wiki/images/6/66/2013-05-02-current-best.png">https://hallcweb.jlab.org/wiki/images/6/66/2013-05-02-current-best.png</a></div><div><br></div><div>If you want to compare them to the same plot, but for spectrometer acceptance bins (aka what I've already been showing), you can find the old plot here: <a href="https://hallcweb.jlab.org/wiki/images/archive/6/66/20130504211619%212013-05-02-current-best.png">https://hallcweb.jlab.org/wiki/images/archive/6/66/20130504211619%212013-05-02-current-best.png</a></div><div><br></div><div>Take care,</div><div>Ellie</div><br><div><div>--------------------------------------------<br>Elena Long, Ph.D.<br></div><div>Post Doctoral Research Associate</div><div>University of New Hampshire</div><div><a href="mailto:elena.long@unh.edu">elena.long@unh.edu</a></div><div><a href="mailto:ellie@jlab.org">ellie@jlab.org</a></div><div><a href="tel:%28603%29%20862-1962">(603) 862-1962</a></div></div><br></div><br>_______________________________________________<br>b1_ana mailing list<br><a href="mailto:b1_ana@jlab.org">b1_ana@jlab.org</a><br><a href="https://mailman.jlab.org/mailman/listinfo/b1_ana">https://mailman.jlab.org/mailman/listinfo/b1_ana</a><br><br></blockquote></div><br></div></blockquote></div><br><div apple-content-edited="true"></div></div><div><div>On May 4, 2013, at 5:34 PM, Karl Slifer <<a href="mailto:karl.slifer@unh.edu">karl.slifer@unh.edu</a>> wrote:</div><br class="Apple-interchange-newline"><blockquote type="cite"><div dir="ltr"><br><div>Hi Ellie,</div><div><br></div><div>great, I know that probably was not very easy to put together quickly.</div><div><br></div><div>Few questions:</div><div><br></div>
<div>-If your assuming W>1.8, I'd move the line in the figure</div><div>-Can you explain what the horizontal lines are in the kin plots?</div><div>-Can you please provide a link to the individual plots for inclusion in the document? </div>
<div>-Also can you point me to the exact values I should put in Table 1 (summary of kinematics)<br></div><div><br></div><div><br></div><div>-Karl</div><div><br></div><div><br></div><div>
<br></div><div><br></div></div><div class="gmail_extra"><br clear="all"><div>---<br><div>Karl J. Slifer<div>Assistant Professor</div><div>University of New Hampshire<br><div>Telephone : <a>603-722-0695</a></div>
</div></div></div>
<br><br><div class="gmail_quote">On Sat, May 4, 2013 at 5:23 PM, Elena Long <<a href="mailto:ellie@jlab.org">ellie@jlab.org</a>> wrote:<br><blockquote class="gmail_quote">
<div><div>Good afternoon,</div><div><br></div><div>As per Oscar's request, I've rebinned the statistical uncertainties into specific x bins. The two highest points contain data from both the SHMS and the HMS. The bins are:</div>
<div><br></div><div>0.09 < 0.16 < 0.23 <br>0.23 < 0.275 < 0.32 <br>0.32 < 0.36 < 0.40 </div><div>0.40 < 0.49 < 0.58 </div><div><br></div><div><div>I've also changed the coloring on dAzz and db1 to black so that they're not confused with the spectrometer acceptance cuts I've been showing previously, and so the PAC doesn't get confused by the colors being similar. </div>
</div><div><br></div><div>The most up-to-date plot including this can be found here: <a href="https://hallcweb.jlab.org/wiki/images/6/66/2013-05-02-current-best.png">https://hallcweb.jlab.org/wiki/images/6/66/2013-05-02-current-best.png</a></div>
<div><br></div><div>If you want to compare them to the same plot, but for spectrometer acceptance bins (aka what I've already been showing), you can find the old plot here: <a href="https://hallcweb.jlab.org/wiki/images/archive/6/66/20130504211619%212013-05-02-current-best.png">https://hallcweb.jlab.org/wiki/images/archive/6/66/20130504211619%212013-05-02-current-best.png</a></div>
<div><br></div><div>Take care,</div><div>Ellie</div><br><div>
<div>
--------------------------------------------<br>Elena Long, Ph.D.<br></div><div>
Post Doctoral Research Associate</div><div>
University of New Hampshire</div><div>
<a href="mailto:elena.long@unh.edu">elena.long@unh.edu</a></div><div>
<a href="mailto:ellie@jlab.org">ellie@jlab.org</a></div><div>
<a href="tel:%28603%29%20862-1962">(603) 862-1962</a></div>
</div>
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<div style="color: rgb(0, 0, 0); font-family: Baskerville; font-size: medium; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; orphans: 2; text-align: -webkit-auto; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; word-wrap: break-word; -webkit-nbsp-mode: space; -webkit-line-break: after-white-space; ">--------------------------------------------<br>Elena Long, Ph.D.<br></div><div style="color: rgb(0, 0, 0); font-family: Baskerville; font-size: medium; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; orphans: 2; text-align: -webkit-auto; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; word-wrap: break-word; -webkit-nbsp-mode: space; -webkit-line-break: after-white-space; ">Post Doctoral Research Associate</div><div style="color: rgb(0, 0, 0); font-family: Baskerville; font-size: medium; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; orphans: 2; text-align: -webkit-auto; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; word-wrap: break-word; -webkit-nbsp-mode: space; -webkit-line-break: after-white-space; ">University of New Hampshire</div><div style="color: rgb(0, 0, 0); font-family: Baskerville; font-size: medium; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; orphans: 2; text-align: -webkit-auto; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; word-wrap: break-word; -webkit-nbsp-mode: space; -webkit-line-break: after-white-space; "><a href="mailto:elena.long@unh.edu">elena.long@unh.edu</a></div><div style="color: rgb(0, 0, 0); font-family: Baskerville; font-size: medium; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; orphans: 2; text-align: -webkit-auto; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; word-wrap: break-word; -webkit-nbsp-mode: space; -webkit-line-break: after-white-space; "><a href="mailto:ellie@jlab.org">ellie@jlab.org</a></div><div style="color: rgb(0, 0, 0); font-family: Baskerville; font-size: medium; font-style: normal; font-variant: normal; font-weight: normal; letter-spacing: normal; line-height: normal; orphans: 2; text-align: -webkit-auto; text-indent: 0px; text-transform: none; white-space: normal; widows: 2; word-spacing: 0px; -webkit-text-size-adjust: auto; -webkit-text-stroke-width: 0px; word-wrap: break-word; -webkit-nbsp-mode: space; -webkit-line-break: after-white-space; ">(603) 862-1962</div>
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