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<u><b>Narbe:</b></u> Looking at plots of E' and (polar)Theta -both
reconstructed- from GEANT-MC to get idea of binning for radiative
corrections<br>
<a class="moz-txt-link-freetext" href="https://hallcweb.jlab.org/experiments/sane/wiki/index.php/SANE_GEANT#05.2F26.2F2010">https://hallcweb.jlab.org/experiments/sane/wiki/index.php/SANE_GEANT#05.2F26.2F2010</a><br>
<br>
Will plot (azimuthal)Phi vs. (polar)Theta in bins of E' as well as
plots of W in bins of Q2<br>
<br>
<br>
<u><b>Jon:</b></u> Supervising an undergrad student to look at
diagnostic histograms for quality checking replay of data set. Will try
to have the undergrad prepare a data-base after finishing.<br>
<br>
<br>
<u><b>Hovhannes:</b></u> Looking at calibrated Q2 vs. x_clust vs.
y_clust to isolate still problematic blocks in BigCal for corrections.
It is from these problematic blocks that very large values of Q2 seem
to be originating and causing negative W2 values. A significant part of
these are from the edges and are consequential of edge-effects.<br>
<br>
<br>
<u><b>Oscar:</b></u> Looking at pi0 mass in cluster energy (E_clust)
bins to check systematics and stability of calibrations. Sees a slight
shift/trend of pi0 mass peak (~16MeV over ~1.3GeV) when he varies
E_clust. Did this for one run (70341). <br>
<a class="moz-txt-link-freetext" href="http://www.jlab.org/~rondon/sane/analysis/replay/pi0/pi0-eclus.gif">http://www.jlab.org/~rondon/sane/analysis/replay/pi0/pi0-eclus.gif</a><br>
<a class="moz-txt-link-freetext" href="http://www.jlab.org/~rondon/sane/analysis/replay/pi0/pi0_mass-eclus_sum.gif">http://www.jlab.org/~rondon/sane/analysis/replay/pi0/pi0_mass-eclus_sum.gif</a><br>
It will be useful to do this for many runs to cover the data
thoroughly. It would also be useful to do this with the MC.<br>
<br>
<br>
As always, please let me know if I missed something or mentioned it
incorrectly.<br>
<br>
Next meeting will be on June 2nd.<br>
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