<html><body><div style="font-family: arial,helvetica,sans-serif; font-size: 12pt; color: #000000"><div>Hi Zulkaida,</div><div><br data-mce-bogus="1"></div><div>I have several comments.</div><div><br data-mce-bogus="1"></div><div>1. add slide numbers</div><div>2. Slide 9. Specify electron beam energy and tagged photon energy range for g9 the same way as you did for g12. For some reason you indicate only maximum.</div><div>3. slide 11. replace "Polarization observable E is the asymmetry between the ω produced when the polarization of the beam and target are symmetries (anti symmetries)." with "Polarization observable E is the asymmetry between the ω produced when the polarization of the beam and target are parallel and antiparallel).</div><div>4. Same slide: "The performed asymmetry is normalized by the degree of the polarization." -> "Measured asymmetry is normalized by the product of beam and target polarizations"</div><div>5. slide 13. Add units (GeV^2) for t axis. Add units for energies. Units for dsigma/dt should be (nb/GeV^2)</div><div><br></div><div data-marker="__SIG_PRE__">-Eugene</div><div><br></div><hr id="zwchr" data-marker="__DIVIDER__"><div data-marker="__HEADERS__"><blockquote style="border-left:2px solid #1010FF;margin-left:5px;padding-left:5px;color:#000;font-weight:normal;font-style:normal;text-decoration:none;font-family:Helvetica,Arial,sans-serif;font-size:12pt;" data-mce-style="border-left: 2px solid #1010FF; margin-left: 5px; padding-left: 5px; color: #000; font-weight: normal; font-style: normal; text-decoration: none; font-family: Helvetica,Arial,sans-serif; font-size: 12pt;"><b>From: </b>"Zulkaida Akbar" <za13@my.fsu.edu><br><b>To: </b>"CLAS Hadron Spectroscopy" <clas_hadron@jlab.org><br><b>Sent: </b>Saturday, January 28, 2017 5:53:22 PM<br><b>Subject: </b>[Clas_hadron] APS April meeting 2017 talk-Zulkaida Akbar<br></blockquote></div><div data-marker="__QUOTED_TEXT__"><blockquote style="border-left:2px solid #1010FF;margin-left:5px;padding-left:5px;color:#000;font-weight:normal;font-style:normal;text-decoration:none;font-family:Helvetica,Arial,sans-serif;font-size:12pt;" data-mce-style="border-left: 2px solid #1010FF; margin-left: 5px; padding-left: 5px; color: #000; font-weight: normal; font-style: normal; text-decoration: none; font-family: Helvetica,Arial,sans-serif; font-size: 12pt;"><div id="divtagdefaultwrapper" style="font-size:12pt;color:#000000;font-family:Calibri,Arial,Helvetica,sans-serif;" dir="ltr" data-mce-style="font-size: 12pt; color: #000000; font-family: Calibri,Arial,Helvetica,sans-serif;"><p>Dear All,</p><p><br></p><p>I will give a talk in APS April meeting about omega photoproduction from FROST and g12. Here is the link to the talk : </p><p><a href="https://clasweb.jlab.org/wiki/images/a/a8/APS_meeting_talk.pdf" class="OWAAutoLink" id="LPlnk389191" target="_blank" data-mce-href="https://clasweb.jlab.org/wiki/images/a/a8/APS_meeting_talk.pdf">https://clasweb.jlab.org/wiki/images/a/a8/APS_meeting_talk.pdf</a><br></p><p><br></p><p>Since this is only 10 minutes talk, I tried to make it very general. Any advice and suggestion would be realy hopeful. Many thanks in advance.</p><p><br></p><p><br></p><p>Best Regard,</p><p><br></p><p>Zulkaida Akbar</p></div><br>_______________________________________________<br>Clas_hadron mailing list<br>Clas_hadron@jlab.org<br>https://mailman.jlab.org/mailman/listinfo/clas_hadron<br></blockquote></div></div></body></html>