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<p>Dear Izzy,</p>
<p>I agree with Volker comments and suggestions. I would also
suggest to change the title into a more general form, for example:</p>
<p><br>
</p>
<p><b>η Electroproduction at CLAS12 </b><br>
</p>
<p><br>
</p>
<p><br>
</p>
<p>All the best</p>
<p>Annalisa<br>
</p>
<div class="moz-cite-prefix">Il 30/06/22 15:21, Volker Burkert ha
scritto:<br>
</div>
<blockquote type="cite"
cite="mid:BLAPR09MB670859D7872986C34DE9DD79C6BA9@BLAPR09MB6708.namprd09.prod.outlook.com">
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<div style="font-family: Calibri, Arial, Helvetica, sans-serif;
font-size: 12pt; color: rgb(0, 0, 0);">
Izzy, </div>
<div style="font-family: Calibri, Arial, Helvetica, sans-serif;
font-size: 12pt; color: rgb(0, 0, 0);">
<br>
</div>
<div style="font-family: Calibri, Arial, Helvetica, sans-serif;
font-size: 12pt; color: rgb(0, 0, 0);">
I would suggest to change the text after "One of the steps ...
". <span style="color: rgb(0, 0, 0); font-family: Calibri,
Arial, Helvetica, sans-serif; font-size: 12pt;"> </span></div>
<div style="font-family: Calibri, Arial, Helvetica, sans-serif;
font-size: 12pt; color: rgb(0, 0, 0);">
<span style="color: rgb(0, 0, 0); font-family: Calibri, Arial,
Helvetica, sans-serif; font-size: 12pt;"><br>
</span></div>
<div style="font-family: Calibri, Arial, Helvetica, sans-serif;
font-size: 12pt; color: rgb(0, 0, 0);">
<span style="caret-color:rgb(0, 0, 0);font-family:"Segoe
UI", "Segoe UI Web (West European)",
"Segoe UI", -apple-system, BlinkMacSystemFont,
Roboto, "Helvetica Neue",
sans-serif;font-size:14.000000953674316px;background-color:rgb(255,
255, 255);display:inline !important">You should mention the
missing mass technique used, and not talk about "eta and eta'
detection", as the final states are NOT "detected" but
"inferred". I don't think you need to detail the binning
procedure and other details.... Your talk will be in the fall
of this year, so you should be beyond the binning process, and
may have some preliminary data to show. Maybe some
unnormalized yields, at least for the eta. I suggest to
de-emphasize the eta' as long as you don't have a definitive
signal. You may say that a similar techniques may be used for
the eta' analysis. </span></div>
<div style="font-family: Calibri, Arial, Helvetica, sans-serif;
font-size: 12pt; color: rgb(0, 0, 0);">
<span style="color: rgb(0, 0, 0); font-family: Calibri, Arial,
Helvetica, sans-serif; font-size: 12pt;"><br>
</span></div>
<div style="color: rgb(0, 0, 0);"><span style="color: rgb(0, 0,
0); font-size: 14.000000953674316px;">Volker</span></div>
<div style="color: rgb(0, 0, 0);"><span style="font-family:
Calibri, Arial, Helvetica, sans-serif; font-size: 12pt; color:
rgb(0, 0, 0);"> </span><br>
</div>
<hr tabindex="-1" style="display:inline-block; width:98%">
<div id="divRplyFwdMsg" dir="ltr"><font style="font-size:11pt"
face="Calibri, sans-serif" color="#000000"><b>From:</b>
Hybrid_baryons <a class="moz-txt-link-rfc2396E" href="mailto:hybrid_baryons-bounces@jlab.org"><hybrid_baryons-bounces@jlab.org></a> on
behalf of Izzy Illari <a class="moz-txt-link-rfc2396E" href="mailto:izzy@jlab.org"><izzy@jlab.org></a><br>
<b>Sent:</b> Wednesday, June 29, 2022 10:35 AM<br>
<b>To:</b> CLAS Hadron <a class="moz-txt-link-rfc2396E" href="mailto:clas_hadron@jlab.org"><clas_hadron@jlab.org></a>;
<a class="moz-txt-link-abbreviated" href="mailto:clas12_rgk@jlab.org">clas12_rgk@jlab.org</a> <a class="moz-txt-link-rfc2396E" href="mailto:clas12_rgk@jlab.org"><clas12_rgk@jlab.org></a>;
<a class="moz-txt-link-abbreviated" href="mailto:hybrid_baryons@jlab.org">hybrid_baryons@jlab.org</a> <a class="moz-txt-link-rfc2396E" href="mailto:hybrid_baryons@jlab.org"><hybrid_baryons@jlab.org></a><br>
<b>Subject:</b> [Hybrid baryons] Abstract for DNP</font>
<div> </div>
</div>
<div>
<p>Dear all,</p>
<p>Copied below is my abstract for this year's DNP for approval.
I would appreciate any comments or contributions. Thank you in
advance for the help.</p>
<p>-title-<br>
Determination of Kinematical Bins for η and η’
Electroproduction with JLab's CLAS12 Detector<br>
-/title-<br>
<br>
-abstract-<br>
The CLAS12 physics program is involved in the studies of the
nucleon resonance spectrum and structure in electroproduction
of a large variety of final states. With new CLAS12 data, we
can investigate the electroproduction of the η and η’ mesons,
which will provide a useful tool to study nucleon resonances
N*. Due to the fact that both η and η’ have isospin I = 0 this
provides an “isospin filter” that allows us to access nucleon
resonances where I = ½. This work uses the 6.5 GeV data
collected by CLAS12, with center of mass energy W ∼ 1-3 GeV,
photon virtuality Q2 ∼ 0-6 GeV2, and luminosity 54 fb-1. The
purpose of this work is to measure the differential cross
section for η and η’ electroproduction. One of the steps
necessary for this measurement is the determination of the
bins and bin sizes for the kinematical parameters W, Q2,
cosθ*, and ϕ*. This will require the development of programs
that filter the data and the application of fiducial cuts to
the remaining final states. After the data has been reduced to
the relevant final states we will develop an automatic method
to fit each individual kinematical bin and determine the
goodness of said fit. This will enable us to extract the η and
η’ signal in each bin to determine which bins can be used and
which will need to be adjusted or rejected. Finally, to verify
η and η’ detection, we will perform Monte Carlo simulations
for comparison. This work is in contrast to the bulk of the
current world database, which focuses on πN final states.<br>
-/abstract-<br>
<br>
</p>
<p>Sincerely,</p>
<p>Izzy<br>
</p>
<pre class="x_moz-signature" cols="72">--
pronouns: they/their/them
Physics Ph.D candidate (Feb 2020)
Columbian College of Arts & Sciences, The George Washington University
M.S. in Physics
The George Washington University (Jan 2020)
B.A. in Physics
Barnard College, Columbia University (May 2017)
GWU Foggy Bottom Office:
Corcoran 418
office phone: (202)994-8896
gwu email: <a href="mailto:iti2103@gwmail.gwu.edu" data-auth="NotApplicable" class="x_moz-txt-link-abbreviated moz-txt-link-freetext" moz-do-not-send="true">iti2103@gwmail.gwu.edu</a>
GWU JLab group
JLab email: <a href="mailto:izzy@jlab.org" data-auth="NotApplicable" class="x_moz-txt-link-abbreviated moz-txt-link-freetext" moz-do-not-send="true">izzy@jlab.org</a>
Personal:
cell: (347)876-4075
email: <a href="mailto:izzyillari@gmail.com" data-auth="NotApplicable" class="x_moz-txt-link-abbreviated moz-txt-link-freetext" moz-do-not-send="true">izzyillari@gmail.com</a></pre>
</div>
<br>
<fieldset class="moz-mime-attachment-header"></fieldset>
<pre class="moz-quote-pre" wrap="">_______________________________________________
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</pre>
</blockquote>
<pre class="moz-signature" cols="72">--
================================================
Prof. Annalisa D'Angelo
Dip. Fisica, Universita' di Roma "Tor Vergata"
Istituto Nazionale di Fisica Nucleare
Sezione di Roma Tor Vergata, Rome Italy
<a class="moz-txt-link-abbreviated" href="mailto:email:annalisa.dangelo@roma2.infn.it">email:annalisa.dangelo@roma2.infn.it</a>
Jefferson Laboratory, Newport News, VA USA
Email: <a class="moz-txt-link-abbreviated" href="mailto:annalisa@jlab.org">annalisa@jlab.org</a>
Tel: + 39 06 72594562
</pre>
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