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Dear Valery,</div>
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thank you very much for your comments and questions.</div>
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I agree with Victors comments regarding the W range and will look into the better notation for the <span style="color: rgb(0, 0, 0); font-size: 18.6667px; background-color: rgb(255, 255, 255); display: inline !important;"><span> </span>$\gamma_vpN^*$.</span></div>
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<span style="color: rgb(0, 0, 0); font-size: 18.6667px; background-color: rgb(255, 255, 255); display: inline !important;">Nick.</span></div>
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<div id="divRplyFwdMsg" dir="ltr"><font face="Calibri, sans-serif" style="font-size:11pt" color="#000000"><b>From:</b> Viktor Mokeev <mokeev@jlab.org><br>
<b>Sent:</b> Monday, January 4, 2021 2:30 PM<br>
<b>To:</b> Valery Kubarovsky <vpk@jlab.org>; Nikolay Markov <markov@jlab.org>; CLAS Hadron <clas_hadron@jlab.org>; Bryan McKinnon <Bryan.McKinnon@glasgow.ac.uk>; Latifa Elouadrhiri <latifa@jlab.org><br>
<b>Subject:</b> Re: APS Meeting abstract</font>
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Dear Valery,</div>
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Previously, the N* region was frequently determined as W<2.0 GeV. However, the extension in the exclusive photoproduction analyses of the last decade increases the value for this limit. </div>
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<div class="x___InlineList__">D.G. Ireland, et al.,<span><span><i> Prog.Part.Nucl.Phys.</i><span> 111</span><span> (2020)</span></span><span> 103752</span></span><span>e-Print:
</span><span><a href="https://arxiv.org/abs/1906.04228" target="_blank" rel="noopener">1906.04228</a><span> [nucl-ex]</span></span></div>
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Another factor which defines this limit is imposed by the capabilities for the credible treatment of the rad correction effects. </div>
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Best Regards,</div>
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Victor<br>
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<div id="x_divRplyFwdMsg" dir="ltr"><font face="Calibri, sans-serif" color="#000000" style="font-size:11pt"><b>From:</b> Clas_hadron <clas_hadron-bounces@jlab.org> on behalf of Valery Kubarovsky <vpk@jlab.org><br>
<b>Sent:</b> Monday, January 4, 2021 2:06 PM<br>
<b>To:</b> Nikolay Markov <markov@jlab.org>; CLAS Hadron <clas_hadron@jlab.org>; Bryan McKinnon <Bryan.McKinnon@glasgow.ac.uk>; Latifa Elouadrhiri <latifa@jlab.org><br>
<b>Subject:</b> Re: [Clas_hadron] APS Meeting abstract</font>
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Dear Nick,</div>
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Where is W<2.5 GeV limit coming from?</div>
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I am not sure that $\gamma_vpN^*$ is the commonly used.</div>
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Best,</div>
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Valery </div>
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<div id="x_x_divRplyFwdMsg" dir="ltr"><font face="Calibri, sans-serif" color="#000000" style="font-size:11pt"><b>From:</b> Clas_hadron <clas_hadron-bounces@jlab.org> on behalf of Nikolay Markov <markov@jlab.org><br>
<b>Sent:</b> Monday, January 4, 2021 13:15<br>
<b>To:</b> CLAS Hadron <clas_hadron@jlab.org>; Bryan McKinnon <Bryan.McKinnon@glasgow.ac.uk>; Latifa Elouadrhiri <latifa@jlab.org><br>
<b>Subject:</b> [Clas_hadron] APS Meeting abstract</font>
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<div style="margin:0px; font-size:12pt; color:black; background-color:white">Dear all,</div>
<div style="margin:0px; font-size:12pt; color:black; background-color:white">attached is my draft for a contributed talk during the upcoming APS meeting at the </div>
<div style="margin:0px; font-size:12pt; color:black; background-color:white"><dt style="background-color:white; color:black">
E8 <span style="margin:0px">Mini-Symposium: Early Science Results from Jefferson Lab 12 GeV Program.</span></dt><dt style="background-color:white; color:black">I will really appreciate your comments and suggestions.</dt><dt style="background-color:white; color:black">Best regards, Nick.</dt></div>
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