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Kyle,<br>
<br>
Well organized talk. Just a few quick comments:<br>
- indicate in the title (first page) that this is trigger hardware
and software<br>
- your pulse form on pages 2 to 5 is not a good representation.
There is only<br>
one clock cycle above the threshold as shown. It does not make good
visual<br>
description of NSB and NSA. We know that NSA>>NSB. Will be
good to<br>
give values to these parameters, it will help to understand the
global picture<br>
- the same for snapshot on page 7 and 8, give a number, I do not
think we <br>
will have too many snapshots in the experiment, it will be 3
probably<br>
- page 16, 17 and 18, what are the thresholds<br>
- the same for picture on page 24/25/26, by the way what is the
difference<br>
between pictures in 24 and 26?<br>
<br>
Stepan<br>
<br>
<div class="moz-cite-prefix">On 4/1/14, 2:27 AM, Kyle McCarty wrote:<br>
</div>
<blockquote
cite="mid:CAPihNJpq=o1hrciOER3M1Ph2AVfdW2JDkGcpjav0w-y=_BLVyw@mail.gmail.com"
type="cite">
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<div>
<div>Hello hps-ecal group,<br>
<br>
</div>
I have attached a prototype for my talk here. It contains a
brief overview the current status of the ecal hardware and the
simulation as well as updated results for background rates and
clustering.triggering. Note that I am going to replace the
clustering/triggering comparisons here with new ones that I am
running now. Currently, I am comparing results from the old
clustering and triggering on the version 4 geometry with the
new algorithms on the version 7 geometry. Since there were
some changes in the rates (especially for the 6.6 GeV data), I
would like to make sure I compare the algorithms using the
same geometry for both.<br>
<br>
</div>
If there are any questions or comments, please feel free to
contact me.<br>
<br>
Thanks,<br>
<br>
Kyle<br>
</div>
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