1
|
Aug 22/24 PionLT/KaonLT Analysis Meeting Notes
|
2
|
----------------------------------------------
|
3
|
(Notes by GH)
|
4
|
|
5
|
Today: KaonLT will be discussed first
|
6
|
|
7
|
Please remember to post your slides at:
|
8
|
https://redmine.jlab.org/projects/kltexp/wiki/Kaon_LT_Meetings
|
9
|
|
10
|
Present
|
11
|
-------
|
12
|
Regina - Garth Huber, Ali Usman, Alicia Postuma, Muhammad Junaid,
|
13
|
Nathan Heinrich, Vijay Kumar, Nacer Hamdi
|
14
|
Virginia - Richard Trotta
|
15
|
JLab - Dave Gaskell
|
16
|
Ohio - Julie Roche
|
17
|
CSULA - Konrad Aniol
|
18
|
|
19
|
Richard
|
20
|
-------
|
21
|
KaonLT Q2=3.0, W=2.32 setting
|
22
|
- HMS-delta shows lots of discrepancies between Data and MC distributions, they
|
23
|
peak in different spots and have markedly different shapes
|
24
|
- HMS-delta vs XPtar, unweighted MC dist fills the same phasespace as the data,
|
25
|
but distribution is much different
|
26
|
- the fact that the filled phasespace has the same shape is good news, so
|
27
|
it's a weighting issue, not something more fundamental
|
28
|
- the MC functional form must be completely inappropriate for these
|
29
|
kinematics
|
30
|
- SHMS-delta vs XPtar, data have a weird banana region at delta~0 that is not
|
31
|
shown in the MC
|
32
|
- data are not pion subtracted, so maybe it's a pi+ leakage issue?
|
33
|
|
34
|
- *NB* it's important to be sure the data dists are clean from pi+ leakage when
|
35
|
making comparo to MC. Next time, please also show a MM plot of the data used
|
36
|
for the distributions, so we can see how much contamination there is.
|
37
|
|
38
|
Nacer
|
39
|
-----
|
40
|
KaonLT Heep Studies
|
41
|
- concentrate on 8.2GeV data, where Exp/MC=1.12
|
42
|
- MM dist shows a small bump at pi0 threshold that needs to be removed
|
43
|
- it would be best if this could be removed with some cut with less
|
44
|
cut-dependence than MM, but that might not be possible
|
45
|
- Ali: *NB* select just the pi0 events with a MM cut and see where they end
|
46
|
up in the other distributions
|
47
|
|
48
|
- the Heep MM distribution is much narrower in MC than Data
|
49
|
- *NB* need to use Ali's resolution tuning result in the MC, so that the MM
|
50
|
distribution gets closer to the data
|
51
|
- probably will eventually need to use a MM>0.10 cut, so it will be important
|
52
|
that the MC more closely resembles the data, to reduce the cut dependence
|
53
|
- *NB* a MM cut dependence study would be required as well
|
54
|
|
55
|
- closer look at the Exp Yield ingredients for this setting
|
56
|
- two notable low effs are EDTM_LT ~89.5% and SHMS_Hodo-3/4 ~97.3%
|
57
|
- concentrate on the EDTM for now
|
58
|
- extracts ElecLT from two methods:
|
59
|
1) ElecLT=EDTM/CPULT 2) calculated from 55ns Hodoscope discriminator width
|
60
|
- method 1:
|
61
|
Run 7974 ElecLT=95.6%, 7975=99.4%, 7976=99.6%
|
62
|
- method 2: some discussion on how to correctly calculate this
|
63
|
- need the total trigger rate from both arms
|
64
|
HMS: ELREAL rate SHMS: 3/4-trigger rate
|
65
|
The total of these two is about 4kHz
|
66
|
- Dave: the Hodoscope discriminator width should always be 55ns, so Method
|
67
|
2 should work the same way for all beam periods, even when the trigger
|
68
|
timing changes
|
69
|
|
70
|
- Dave: *NB* please compare the beam current for these 3 runs and the %time
|
71
|
that the beam current is over threshold, so we can better understand the
|
72
|
variation between run 7974 and the others
|
73
|
|
74
|
- plots shown of HMS-delta and SHMS-delta vs MM
|
75
|
- the Heep data distribution has a blob on one end while the MC distribution
|
76
|
is more uniform
|
77
|
- this blob can't be due to pi0 contamination, since it occurs at elastic MM
|
78
|
|
79
|
- *NB* also need to investigate use of different HMS-Matrix Element for
|
80
|
intermediate momenta, as suggested last week
|
81
|
- *NB* setting up an offline meeting on this w/ Dave would be a good idea
|
82
|
|
83
|
Junaid
|
84
|
------
|
85
|
PionLT Heep study
|
86
|
- 2022 data had a broader EM distribution than others
|
87
|
- fixed raster correction, dists now sharper, more similar to 2021 data
|
88
|
- extracted new mean values and gave to GH for Offset Fitting
|
89
|
|
90
|
- looking at efficiencies to better understand non-unity Exp/MC ratios
|
91
|
- SHMS_Hodo-3/4 effis are low ~89%
|
92
|
- Plane-by-Plane efficiencies show a decreasing efficiency with plane
|
93
|
number
|
94
|
- Plane 4 (the quartz bars) has an eff of only ~61%
|
95
|
- *NB* suggest to look at efficiencies vs rate, if it is real there will be
|
96
|
correlation, if it is something else, it will be more random
|
97
|
|
98
|
- also looking at pi0 contamination study, given Nacer's findings
|
99
|
|
100
|
Ali, Alicia, Vijay
|
101
|
------------------
|
102
|
- no reports
|
103
|
- congratulations to Vijay on the successful PhD defense!
|
104
|
|
105
|
Future Meetings
|
106
|
---------------
|
107
|
- the current time will not be good for both Julie and Nacer due to conflict
|
108
|
with teaching
|
109
|
- Julie will be available at 4pm and 11am Eastern
|
110
|
- GH will set up a poll to find a new time, starting in September
|
111
|
|
112
|
Next Meeting
|
113
|
-------------
|
114
|
- Thur Aug 29 @ 15:00 Eastern/13:00 Regina
|
115
|
- PionLT will go first
|
116
|
|
117
|
|
118
|
|