[Halld-pid] Start Counter Meeting Minutes, April 16, 2020
Mark Ito
marki at jlab.org
Sun Apr 19 12:39:46 EDT 2020
Folks,
Please find the minutes here
<https://halldweb.jlab.org/wiki/index.php/GlueX_Start_Counter_Meeting,_April_16,_2020#Minutes>
and below.
-- Mark
GlueX Start Counter Meeting, April 16, 2020, Minutes
Present: Rupesh Dotel, Tolga Erbora, Mark Ito, Simon Taylor, Beni Zihlmann
There is a recording of this meeting <https://bluejeans.com/s/us4VA/> on
the BlueJeans site. Use your JLab credentials to gain access.
Review of minutes from the last meeting
We went over the minutes from April 2
<https://halldweb.jlab.org/wiki/index.php/GlueX_Start_Counter_Meeting,_April_2,_2020#Minutes>
without significant comment.
Calibration and Efficiency
Rupesh is working on documenting the calibration procedures that he
worked so hard to get going before it fades from memory. He is also
thinking about a plan for doing some calibrations for the run just past
at appropriate intervals.
Dark Rate Studies
Beni showed plot of the dark rate effects using a new method. Rather
using the result from FPGA-providided pedestal measurement, he sums all
of the data in the readout window in raw mode to assess pedestal the
pedestal value. He has also changed the fit method. Rather than just
fitting the low-side of the pedestal distribution to a Gaussian, he
constrains the amplitude and the position of the Gaussian peak to within
a narrow range around the peak of the pedestal distribution. He showed
two plots. On the left is the old method, and the right the new.
<https://halldweb.jlab.org/wiki/index.php/File:Sctest_pedestals.png>
Old Method
<https://halldweb.jlab.org/wiki/index.php/File:Sctest_usesamples.png>
New Method
We noted that even though the methods are quite a bit different, the
trendline and size of the effect are the same.
Tolga has been trying to reproduce Beni's result (old method). He is
ready to averate the results of the 30 start counter paddles got get a
single plot.
Actin Item Review
1. Document calibration procedure (Rupesh)
2. Obtained calibrations for sub-periods of the recent run. (Rupesh)
3. Reproduce Beni's dark current results. (Tolga)
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* This page was last modified on 19 April 2020, at 12:37.
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