<html><head><meta http-equiv="Content-Type" content="text/html charset=us-ascii"></head><body style="word-wrap: break-word; -webkit-nbsp-mode: space; -webkit-line-break: after-white-space;" class="">Dear Annalisa,<div class="">will start today.</div><div class="">Nick.<br class=""><div><blockquote type="cite" class=""><div class="">On Aug 20, 2019, at 5:20 AM, Annalisa D'Angelo <<a href="mailto:annalisa.dangelo@roma2.infn.it" class="">annalisa.dangelo@roma2.infn.it</a>> wrote:</div><br class="Apple-interchange-newline"><div class="">
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<div text="#000000" bgcolor="#FFFFFF" class=""><p class="">Dear Nick, Dear Raffaella,<br class="">
</p><p class="">thank you!</p><p class="">I understand that sub-systems calibration is completed.<br class="">
</p><p class="">At this point I propose to go for pass0: would you please decode
and cook 10 files for each good run in the rg-k range: 5694 -
6000.</p><p class="">Annalisa<br class="">
</p><p class=""><br class="">
</p>
<div class="moz-cite-prefix">Il 19/08/19 17:42, markov ha scritto:<br class="">
</div>
<blockquote type="cite" cite="mid:13EC4D1D-9CEA-408E-9EC2-347190EC62B5@jlab.org" class="">
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Dear Annalisa,
<div class="">I have updated spreadsheets with the new
calibrations (RGA and RGK are now separated):</div>
<div class=""><a href="https://urldefense.proofpoint.com/v2/url?u=https-3A__docs.google.com_spreadsheets_d_1x-5F7N-5FIYjsAm-5FpVS4PBg2MQLOyc8HOfOr9pdUPCMcbe0_edit-23gid-3D0&d=DwMD-g&c=CJqEzB1piLOyyvZjb8YUQw&r=xciK_tm-6s3sa3rNEPqgUg&m=qPwPjUcqzh6PMnz7VIZQcMS5IqSS3bPbpLJ_9BCFf8k&s=mSS2D2VG_e0N5ah9SZ8ZKy5pz8BeLJPpVv8nlcyWQjc&e=" class="" moz-do-not-send="true">https://docs.google.com/spreadsheets/d/1x_7N_IYjsAm_pVS4PBg2MQLOyc8HOfOr9pdUPCMcbe0/edit#gid=0</a></div>
<div class="">Raffaella updated the FT. Is there is anything we
need?</div>
<div class="">Nick. <br class="">
<div class="">
<blockquote type="cite" class="">
<div class="">On Aug 17, 2019, at 1:56 PM, markov <<a href="mailto:markov@jlab.org" class="" moz-do-not-send="true">markov@jlab.org</a>> wrote:</div>
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<div class="">
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charset=windows-1252" class="">
<div style="word-wrap: break-word; -webkit-nbsp-mode:
space; -webkit-line-break: after-white-space;" class="">Sorry,
I have sent update to Raffaella only:
<div class="">they were cooked, the file location is:</div>
<div class="">
<div style="margin: 0px; line-height: normal;
font-family: Courier; color: rgb(255, 240, 165);
background-color: rgb(19, 119, 61);" class=""><span style="font-variant-ligatures:
no-common-ligatures" class="">/volatile/clas12/rg-k/production/recon/pass0/calib/v13/</span></div>
<div class="">
<blockquote type="cite" class="">
<div class="">On Aug 17, 2019, at 5:28 AM,
Annalisa D'Angelo <<a href="mailto:annalisa.dangelo@roma2.infn.it" class="" moz-do-not-send="true">annalisa.dangelo@roma2.infn.it</a>>
wrote:</div>
<br class="Apple-interchange-newline">
<div class="">
<div class="">Dear Nick,<br class="">
<br class="">
any update on the cooking of two more runs for
Raffaella?<br class="">
<br class="">
I understand we are waiting for them to
complete the RG-K calibration at this step....<br class="">
<br class="">
Thank you for your help<br class="">
<br class="">
Annalisa<br class="">
<br class="">
Il 14/08/19 14:23, markov ha scritto:<br class="">
<blockquote type="cite" class="">Dear
Annalisa,<br class="">
just a quick update, files have been decoded
recently, I will submit them for the
reconstruction right after First experiment
meeting.<br class="">
I am sorry for the delay, Nick.<br class="">
<blockquote type="cite" class="">On Aug 14,
2019, at 8:12 AM, markov <<a href="mailto:markov@jlab.org" class="" moz-do-not-send="true">markov@jlab.org</a>>
wrote:<br class="">
<br class="">
Dear Annalisa,<br class="">
I am decoding corresponding files, this
should be finished soon.<br class="">
Sorry for the delay.<br class="">
Nick.<br class="">
<blockquote type="cite" class="">On Aug
14, 2019, at 6:01 AM, Annalisa D'Angelo
<<a href="mailto:annalisa.dangelo@roma2.infn.it" class="" moz-do-not-send="true">annalisa.dangelo@roma2.infn.it</a>>
wrote:<br class="">
<br class="">
Dear Nick and Will,<br class="">
<br class="">
have two more runs from RG-K at 7.5 GeV
cooked for Rafafella's FT calibration?<br class="">
<br class="">
Thank you<br class="">
<br class="">
Annalisa<br class="">
<br class="">
Il 09/08/19 15:54, markov ha scritto:<br class="">
<blockquote type="cite" class="">Dear
all,<br class="">
sure I will submit two more runs.<br class="">
Nick.<br class="">
<blockquote type="cite" class="">On
Aug 9, 2019, at 9:51 AM, Raffaella
De Vita <<a href="mailto:Raffaella.Devita@ge.infn.it" class="" moz-do-not-send="true">Raffaella.Devita@ge.infn.it</a>>
wrote:<br class="">
<br class="">
Dear Annalisa,<br class="">
I ran FT calibrations on run 5700
but for the energy calibrations I
would benefit from having more
statistics: would it be possible to
have another two runs cooked close
to 5700?<br class="">
Thanks,<br class="">
<span class="Apple-tab-span" style="white-space:pre"> </span>Raffaella<br class="">
<br class="">
<blockquote type="cite" class="">On
30 Jul 2019, at 04:44, Annalisa
D'Angelo <<a href="mailto:annalisa.dangelo@roma2.infn.it" class="" moz-do-not-send="true">annalisa.dangelo@roma2.infn.it</a>>
wrote:<br class="">
<br class="">
Dear All,<br class="">
<br class="">
you may find the skimmed and
filtered trains here:<br class="">
<br class="">
/w/hallb-scifs17exp/clas12/rg-k/trains/calibration/v13<br class="">
<br class="">
(/work/clas12/rg-k/trains/calibration/v13)<br class="">
<br class="">
Previous link was to cooked
files...<br class="">
<br class="">
All the best<br class="">
<br class="">
Annalisa<br class="">
<br class="">
Il 30/07/19 07:56, Annalisa
D'Angelo ha scritto:<br class="">
<blockquote type="cite" class="">Dear
All,<br class="">
<br class="">
the RGK 5700 5893 have been
calibrated for the FTOF and have
been re-cooked. They are ready
to be calibrated for the
following detectors:<br class="">
<br class="">
CND<br class="">
<br class="">
HTCC<br class="">
<br class="">
LTCC<br class="">
<br class="">
RICH<br class="">
<br class="">
FT<br class="">
<br class="">
RF<br class="">
<br class="">
SVT<br class="">
<br class="">
You may find the skimmed and
filtered trains at:<br class="">
<br class="">
/lustre/expphy/volatile/clas12/rg-k/production/recon/calib/v13/005893<br class="">
<br class="">
/lustre/expphy/volatile/clas12/rg-k/production/recon/calib/v13/005700<br class="">
<br class="">
Please proceed with the detector
calibration you are in charge of
at your earliest convenience.<br class="">
<br class="">
Thank you<br class="">
<br class="">
Annalisa<br class="">
<br class="">
p.s. DC and CTOF have already
been calibrated on the same
files.<br class="">
<br class="">
p.p.s Files have been cooked
using version 6b.3.0.<br class="">
<br class="">
</blockquote>
-- <br class="">
================================================<br class="">
Prof. Annalisa D'Angelo<br class="">
Dip. Fisica, Universita' di Roma
"Tor Vergata"<br class="">
INFN Sezione di Roma Tor Vergata,
Rome Italy<br class="">
email:<a href="mailto:annalisa.dangelo@roma2.infn.it" class="" moz-do-not-send="true">annalisa.dangelo@roma2.infn.it</a><br class="">
Jefferson Laboratory, Newport
News, VA USA<br class="">
Email: <a href="mailto:annalisa@jlab.org" class="" moz-do-not-send="true">annalisa@jlab.org</a><br class="">
Tel: + 39 06 72594562<br class="">
<br class="">
<br class="">
<br class="">
</blockquote>
</blockquote>
</blockquote>
-- <br class="">
================================================<br class="">
Prof. Annalisa D'Angelo<br class="">
Dip. Fisica, Universita' di Roma "Tor
Vergata"<br class="">
INFN Sezione di Roma Tor Vergata, Rome
Italy<br class="">
email:<a href="mailto:annalisa.dangelo@roma2.infn.it" class="" moz-do-not-send="true">annalisa.dangelo@roma2.infn.it</a><br class="">
Jefferson Laboratory, Newport News, VA
USA<br class="">
Email: <a href="mailto:annalisa@jlab.org" class="" moz-do-not-send="true">annalisa@jlab.org</a><br class="">
Tel: + 39 06 72594562<br class="">
<br class="">
<br class="">
</blockquote>
</blockquote>
<br class="">
</blockquote>
-- <br class="">
================================================<br class="">
Prof. Annalisa D'Angelo<br class="">
Dip. Fisica, Universita' di Roma "Tor Vergata"<br class="">
INFN Sezione di Roma Tor Vergata, Rome Italy<br class="">
email:<a href="mailto:annalisa.dangelo@roma2.infn.it" class="" moz-do-not-send="true">annalisa.dangelo@roma2.infn.it</a><br class="">
Jefferson Laboratory, Newport News, VA USA<br class="">
Email: <a href="mailto:annalisa@jlab.org" class="" moz-do-not-send="true">annalisa@jlab.org</a><br class="">
Tel: + 39 06 72594562<br class="">
<br class="">
<br class="">
</div>
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</blockquote>
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</blockquote>
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<br class="">
</div>
</blockquote>
<pre class="moz-signature" cols="72">--
================================================
Prof. Annalisa D'Angelo
Dip. Fisica, Universita' di Roma "Tor Vergata"
INFN 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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