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<div class="moz-cite-prefix">Hi Marco,<br>
<br>
I tried the same on the run and channels you sent. And found
similar results - but I think it is because the old filtering we
used subsets of 32 channels and in the new code today i saw it is
set up for subsets of 8 pixels. So then i re-ran after changing in
TBlock.cpp to subsets of 32 and got back the same. Please see
attached.<br>
<br>
run300_chan4000_FilterAndEvList_Subset32.png = new combined
filtering and event matching with filter subset 32<br>
run300_chan4000_FilterAndEvList.png = new combined filtering and
event matching with filter subset 8<br>
run300_chan4000_Filter.png = old parsing, only filter no event
matching subset 32<br>
<br>
Thanks,<br>
Rachel<br>
<br>
On 22/10/12 16:21, mirazita wrote:<br>
</div>
<blockquote cite="mid:362eecb08e684dab1c5b94c4f3c0ee38@lnf.infn.it" type="cite">
<pre wrap="">Hi all,
I tried to re-parse the run 300 data but I found some difference in the
Maroc with respect to the old code, see the attached plots for channel
4000.
Did anybody else find the same?
Marco
On Fri, 19 Oct 2012 20:03:26 +0200, Evaristo Cisbani
<a href="mailto:evaristo.cisbani@iss.infn.it"><evaristo.cisbani@iss.infn.it></a> wrote:
</pre>
<blockquote type="cite">
<pre wrap="">Dear All,
attached are the files that merge the common noise filtering coded by
Matteo and the generation of the "good" TEventList.
Please check it and let me know if there are problems.
Evaristo
On Fri, 2012-10-19 at 18:09 +0200, Marco Mirazita wrote:
</pre>
<blockquote type="cite">
<pre wrap="">I have put in my directory at jlab the new software for the binary file
</pre>
</blockquote>
</blockquote>
<pre wrap="">
</pre>
<blockquote type="cite">
<blockquote type="cite">
<pre wrap="">conversion:
1) /w/hallb/infn2/mirazita/TEST_CERN2012/apv/analysis/
has the TEventList stuff but not the common noise filtering
2) /w/hallb/infn2/mirazita/TEST_CERN2012/apv/analysis_CNS/
has the common noise filtering but not the TEventList.
You should run 1) first, take the root file with the TEventList and
</pre>
</blockquote>
</blockquote>
<pre wrap="">then
</pre>
<blockquote type="cite">
<blockquote type="cite">
<pre wrap="">run 2) to obtain the GEM and MAROC root data. Please note that in the
previous code in 2) there was a bug (the event number in the MAROC part
</pre>
</blockquote>
</blockquote>
<pre wrap="">
</pre>
<blockquote type="cite">
<blockquote type="cite">
<pre wrap="">was wrong for some reason), so you should regenerate the root files.
Hopefully we will have soon one version of the code doing everithing.
Marco
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<pre wrap="">_______________________________________________
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</pre>
</blockquote>
</blockquote>
</blockquote>
<br>
<br>
<pre class="moz-signature" cols="72">--
Rachel Montgomery
Nuclear Physics Group
School of Physics and Astronomy
Kelvin Building, Room 407
University of Glasgow
Glasgow
G12 8QQ
Scotland
Tel: +44 (0)141 330 6398
</pre>
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