<html>
<head>
<meta http-equiv="Content-Type" content="text/html; charset=us-ascii">
<style type="text/css" style="display:none;"> P {margin-top:0;margin-bottom:0;} </style>
</head>
<body dir="ltr">
<div class="elementToProof" style="font-family: Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
Haiyun,</div>
<div class="elementToProof" style="font-family: Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
<br>
</div>
<div class="elementToProof" style="font-family: Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
I have some questions/comments about the most recent</div>
<div class="elementToProof" style="font-family: Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
analysis note.</div>
<div class="elementToProof" style="font-family: Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">
<br>
</div>
<ol data-editing-info="{"orderedStyleType":4,"unorderedStyleType":1}" style="margin-block: 0px;">
<li style="list-style-type: "(1) ";">
<div style="color: rgb(0, 0, 0); font-family: Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif; font-size: 12pt;">
<span style="font-family: Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">In Figure 32, G vs cos(theta) plots for the W = 1860</span></div>
<div style="color: rgb(0, 0, 0); font-family: Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif; font-size: 12pt;">
<span style="font-family: Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">and 1940 seem to be the identical.</span></div>
<div style="color: rgb(0, 0, 0); font-family: Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif; font-size: 12pt;">
<span style="font-family: Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);"><br>
</span></div>
<div style="color: rgb(0, 0, 0); font-family: Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif; font-size: 12pt;">
<span style="font-family: Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif; font-size: 12pt; color: rgb(0, 0, 0);">(2) Numbers from fit values at Fig. 38, for example,</span></div>
<div><font color="#000000" face="Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif" size="3">seem to </font><font color="#000000" face="Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif"><span style="caret-color: rgb(0, 0, 0);">different</span></font><font color="#000000" face="Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif" size="3"> from those
on the table.10.</font></div>
<div><font color="#000000" face="Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif" size="3"><br>
</font></div>
<div><font color="#000000" face="Aptos, Aptos_EmbeddedFont, Aptos_MSFontService, Calibri, Helvetica, sans-serif" size="3">Regards, Tsuneo Kageya. </font></div>
</li></ol>
<div id="appendonsend"></div>
<hr style="display:inline-block;width:98%" tabindex="-1">
<div id="divRplyFwdMsg" dir="ltr"><font face="Calibri, sans-serif" style="font-size:11pt" color="#000000"><b>From:</b> G14_run <g14_run-bounces@jlab.org> on behalf of g14_run-request@jlab.org <g14_run-request@jlab.org><br>
<b>Sent:</b> Wednesday, February 7, 2024 10:58 AM<br>
<b>To:</b> g14_run@jlab.org <g14_run@jlab.org><br>
<b>Subject:</b> G14_run Digest, Vol 149, Issue 6</font>
<div> </div>
</div>
<div class="BodyFragment"><font size="2"><span style="font-size:11pt;">
<div class="PlainText">Send G14_run mailing list submissions to<br>
g14_run@jlab.org<br>
<br>
To subscribe or unsubscribe via the World Wide Web, visit<br>
<a href="https://mailman.jlab.org/mailman/listinfo/g14_run">https://mailman.jlab.org/mailman/listinfo/g14_run</a><br>
or, via email, send a message with subject or body 'help' to<br>
g14_run-request@jlab.org<br>
<br>
You can reach the person managing the list at<br>
g14_run-owner@jlab.org<br>
<br>
When replying, please edit your Subject line so it is more specific<br>
than "Re: Contents of G14_run digest..."<br>
<br>
<br>
Today's Topics:<br>
<br>
1. [EXTERNAL] Reminder: g14 meeting tomorrow at 9:00 am JLab<br>
time (Annalisa.Dangelo@roma2.infn.it)<br>
2. [EXTERNAL] Today's g14 meeting (Annalisa.Dangelo@roma2.infn.it)<br>
<br>
<br>
----------------------------------------------------------------------<br>
<br>
Message: 1<br>
Date: Tue, 6 Feb 2024 19:18:29 +0100 (CET)<br>
From: "Annalisa.Dangelo@roma2.infn.it" <annalisa@roma2.infn.it><br>
To: g14 run <g14_run@jlab.org>, Haiyun Lu <haiyun.lu@gmail.com>,<br>
Tsuneo Kageya <kageya@jlab.org><br>
Subject: [G14_run] [EXTERNAL] Reminder: g14 meeting tomorrow at 9:00<br>
am JLab time<br>
Message-ID:<br>
<235701868.147509.1707243509405.JavaMail.zimbra@roma2.infn.it><br>
Content-Type: text/plain; charset="utf-8"<br>
<br>
<br>
<br>
Dear All, <br>
<br>
this is a reminder of tomorrow g14 meeting at 9:00 am JLab time. <br>
<br>
The link to the Zoom meeting is the following: <br>
<br>
[ <a href="https://urldefense.proofpoint.com/v2/url?u=https-3A__jlab-2Dorg.zoomgov.com_j_1608547947-3Fpwd-3DM1ZRc3k1dTlWek1Tb1o3V25uWlN1Zz09&d=DwMFaQ&c=CJqEzB1piLOyyvZjb8YUQw&r=5LSWsFN5KweowPCsdwCuT6TNyYmHKJ3RcKK8qa-oO-g&m=a5rjQAEeKmo8bQtcVy3QdyKUoET0we9Jt90VgYZE6f5cVzmGbAKur5SnZuc9MtqW&s=qL3Z8lhB8Nm9KfOxpgaaYb7k-RjuLS1_ioAftn0b57w&e=">
https://urldefense.proofpoint.com/v2/url?u=https-3A__jlab-2Dorg.zoomgov.com_j_1608547947-3Fpwd-3DM1ZRc3k1dTlWek1Tb1o3V25uWlN1Zz09&d=DwMFaQ&c=CJqEzB1piLOyyvZjb8YUQw&r=5LSWsFN5KweowPCsdwCuT6TNyYmHKJ3RcKK8qa-oO-g&m=a5rjQAEeKmo8bQtcVy3QdyKUoET0we9Jt90VgYZE6f5cVzmGbAKur5SnZuc9MtqW&s=qL3Z8lhB8Nm9KfOxpgaaYb7k-RjuLS1_ioAftn0b57w&e=</a>
| <a href="https://urldefense.proofpoint.com/v2/url?u=https-3A__jlab-2Dorg.zoomgov.com_j_1608547947-3Fpwd-3DM1ZRc3k1dTlWek1Tb1o3V25uWlN1Zz09&d=DwIFaQ&c=CJqEzB1piLOyyvZjb8YUQw&r=5LSWsFN5KweowPCsdwCuT6TNyYmHKJ3RcKK8qa-oO-g&m=80zpNA4HE7t4MWtJQ3ZQJlOLF4I3KdVt7T3YJjAG6jLyOzvqbdMpqkdTStsATWuQ&s=n_Wo-1Wc0SBDfS6XtD3FxX0Vu2pfJVAeoNi0KSC9XRY&e=">
https://urldefense.proofpoint.com/v2/url?u=https-3A__jlab-2Dorg.zoomgov.com_j_1608547947-3Fpwd-3DM1ZRc3k1dTlWek1Tb1o3V25uWlN1Zz09&d=DwIFaQ&c=CJqEzB1piLOyyvZjb8YUQw&r=5LSWsFN5KweowPCsdwCuT6TNyYmHKJ3RcKK8qa-oO-g&m=80zpNA4HE7t4MWtJQ3ZQJlOLF4I3KdVt7T3YJjAG6jLyOzvqbdMpqkdTStsATWuQ&s=n_Wo-1Wc0SBDfS6XtD3FxX0Vu2pfJVAeoNi0KSC9XRY&e=</a>
] <br>
<br>
<br>
meeting id is <br>
160 854 7947 <br>
<br>
<br>
<br>
if required passcode is <br>
<br>
<br>
396000. <br>
All the best <br>
Annalisa <br>
Prof.ssa Annalisa D'Angelo <br>
Dip Fisica Universit? di Roma Tor Vergata e INFN Roma Tor Vergata <br>
Jefferson Lab <br>
-------------- next part --------------<br>
An HTML attachment was scrubbed...<br>
URL: <<a href="https://mailman.jlab.org/pipermail/g14_run/attachments/20240206/f467084d/attachment-0001.html">https://mailman.jlab.org/pipermail/g14_run/attachments/20240206/f467084d/attachment-0001.html</a>><br>
<br>
------------------------------<br>
<br>
Message: 2<br>
Date: Wed, 7 Feb 2024 16:58:47 +0100 (CET)<br>
From: "Annalisa.Dangelo@roma2.infn.it" <annalisa@roma2.infn.it><br>
To: Haiyun Lu <haiyun.lu@gmail.com><br>
Cc: g14 run <g14_run@jlab.org>, Tsuneo Kageya <kageya@jlab.org><br>
Subject: [G14_run] [EXTERNAL] Today's g14 meeting<br>
Message-ID:<br>
<1392035994.62365.1707321527983.JavaMail.zimbra@roma2.infn.it><br>
Content-Type: text/plain; charset="utf-8"<br>
<br>
Dear Haiyun, <br>
we have revised the results reported in the present version of the analysis note and we have realized that the fluctuations of Gsin(phi) data are now spanning in ranges that are way larger that the physical [-1;1] range.
<br>
As a consequence the statistical errors of the extracted G values have huge relative errors.
<br>
The present results do not carry information that may be published. <br>
The next step we have decided to take is to double check again the numbers and the formulas:
<br>
- we may use the tables you have sent last december or the yields obtained by Tsuneo in the same bins, and apply the formulas you have reported in the analysis note or the formulas used by Tsuneo; we could obtain 4 different distributions for Gsin2phi (and
4 different distributions for Sigma cos2phi) for each W,theta bin. <br>
We hope to get a better understanding of the results from the comparison of the 4 versions of the same distribution.
<br>
One last question: we have noticed that some of the yield values are equal to zero.
<br>
What did you do with those values? Did you discard the points or are they used in the fit?
<br>
We are planning to hold next g14 meeting in two weeks. <br>
All the best <br>
Annalisa <br>
-------------- next part --------------<br>
An HTML attachment was scrubbed...<br>
URL: <<a href="https://mailman.jlab.org/pipermail/g14_run/attachments/20240207/5aec988e/attachment.html">https://mailman.jlab.org/pipermail/g14_run/attachments/20240207/5aec988e/attachment.html</a>><br>
<br>
------------------------------<br>
<br>
Subject: Digest Footer<br>
<br>
_______________________________________________<br>
G14_run mailing list<br>
G14_run@jlab.org<br>
<a href="https://mailman.jlab.org/mailman/listinfo/g14_run">https://mailman.jlab.org/mailman/listinfo/g14_run</a><br>
<br>
<br>
------------------------------<br>
<br>
End of G14_run Digest, Vol 149, Issue 6<br>
***************************************<br>
</div>
</span></font></div>
</body>
</html>