1
|
Octt 3/23 PionLT/KaonLT Analysis Meeting Notes
|
2
|
----------------------------------------------
|
3
|
(Notes by GH, AH & RT)
|
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 - Alicia Postuma, Muhammad Junaid, Nacer Hamdi, Nathan Heinrich,
|
13
|
Vijay Kumar, Garth Huber
|
14
|
CUA - Richard Trotta
|
15
|
FIU - Pete Markowitz
|
16
|
|
17
|
Richard
|
18
|
-------
|
19
|
Q2=2.1 R=Data/SIMC plots vs phi for t-bins at low, high epsilon
|
20
|
- Sync the range of angles between SIMC [0, 2Pi] and hcana [-Pi, Pi]
|
21
|
- added pi to hcana phi
|
22
|
- high ratios at phi=240,280 deg consistently for all 3 t-bins, SIMC events go
|
23
|
to zero for these bins
|
24
|
- unweighted distributions show events in these bins, so it is presumably a
|
25
|
weighting issue
|
26
|
- sigTT is calculated way too large for some bins as well
|
27
|
|
28
|
- using starting parameters from LD+ Fpi-2 analysis
|
29
|
- no changes to t-average calculation yet
|
30
|
- m_pi pole factor not yet modified for m_K
|
31
|
- no (Q2,W) scaling appiled yet to leading parameters
|
32
|
- this may solve the issue, the important thing is to estimate a set of
|
33
|
initial starting parameters that behave reasonably, Richard will need to
|
34
|
do a by-hand calculation to find them
|
35
|
|
36
|
Some high epsilon data have two slightly different TH_shms, e.g. some right
|
37
|
setting data were taken initially and came back to take more statistics later,
|
38
|
the TH_shms differ slightly between the two sets
|
39
|
- Garth: for the experimental data, need to select the right angle for each run
|
40
|
number in standard.kinematics
|
41
|
- for SIMC, if the difference is small (typically 0.005deg), run SIMC using
|
42
|
the mean angle of the data (weighted by the accumulated beam charge)
|
43
|
|
44
|
Still running Heep for offset check
|
45
|
- getting ifarm replay errors: SLURM FAIL
|
46
|
- Nathan also has ifarm issues since Friday
|
47
|
- will follow up with IT tomorrow
|
48
|
|
49
|
|
50
|
Vijay
|
51
|
-----
|
52
|
Sent Heep plots for new offsets to GH yesterday
|
53
|
- looking at comparison of tar and spectrometer variables between data and SIMC
|
54
|
after reconstruction script
|
55
|
|
56
|
Lumi studies will start son
|
57
|
- low current BCM calibs are very important to the low Q2 data!
|
58
|
|
59
|
Nathan
|
60
|
------
|
61
|
Hodscope calibration ongoing (V_prop 2021 data)
|
62
|
- met w/Junaid to explain the calibration process
|
63
|
- batch errors lead to slowing calibration jobs
|
64
|
|
65
|
Junaid
|
66
|
------
|
67
|
Helping Nathan with Hosdoscope calibration (V_prop 2022 data)
|
68
|
- was using Stephen's old scripts, now switched to new scripts
|
69
|
- one of the points of NH and MJ work is that we don't know how many different
|
70
|
sets of V_prop will be needed, so need to calibrate a selection of all data
|
71
|
to study parameter stability
|
72
|
- V_prop is a whole matrix, so many more parameters than time offsets
|
73
|
- using interactive so far for script testing, so not yet delayed by ifarm
|
74
|
issues
|
75
|
|
76
|
Alicia
|
77
|
------
|
78
|
HGC vs. Aerogel Cherenkov NPE (10.6 GeV data)
|
79
|
- Noticed negative NPE in the HGC!
|
80
|
- 2D plot of HGC vs Aero
|
81
|
- events w/ HGC npe<0 but Aero having 5-20 npe
|
82
|
- needs some investigation of the HGC calibration for these runs
|
83
|
|
84
|
- Vijay quickly confirms that HGC calibrations for 10.6 GeV data were done for
|
85
|
runs 4875-5325
|
86
|
- first step is for Alicia to confirm that she is using the correct
|
87
|
calibration files
|
88
|
|
89
|
Nacer
|
90
|
-----
|
91
|
- going through event selection & variables for low Q2 KaonLT data
|
92
|
|
93
|
---------------------------------------------------------------------
|
94
|
Post-Meeting on CoinTime leakage in 10.6GeV KaonLT data
|
95
|
- Dave, Richard, Alicia, Junaid, Nacer, Vijay, GH
|
96
|
|
97
|
Alicia shows plot of CT (range -30,30+log z) vs MM (pi+n PID)
|
98
|
- mmpi_10p6.pdf
|
99
|
- see a band with good pi+ MM over a wide range of CT
|
100
|
- the behavior is atypical, but could be due to poor CT timing resolution
|
101
|
during 10.6GeV run, which was fortunately fixed before rest of KaonLT run
|
102
|
- Nacer confirmed at Regina group meeting that this behavior is absent in 3.8
|
103
|
GeV data, no CT band at pi+n mass
|
104
|
|
105
|
- Dave: Why is the band not through whole region?
|
106
|
- Should be at other MM peaks (ie K+lambda)
|
107
|
- Is it just because pi+n is so large, and harder to see in lambda?
|
108
|
- this is most likely the case, Alicia changes some cuts to select
|
109
|
pi+Delta region and the problem seems to be there too, although more
|
110
|
washed out in MM
|
111
|
|
112
|
- Dave: can have singles within cointime window and steal the good time
|
113
|
(making it show up at bad time) although the tracking algorithm still picks
|
114
|
up the correct MM
|
115
|
- In general, this should have a very small probability, unless timing
|
116
|
window cuts are wide open
|
117
|
- need to treat CoinTime like any other detector and place time windows on
|
118
|
both legs into CoinTime module
|
119
|
|
120
|
Richard confirms that Timing windows for KaonLT hallc_replay are set:
|
121
|
github.com/JeffersonLab/hallc_replay_lt/blob/LTSep_Analysis_2022/PARAM/
|
122
|
TRIG/KaonLT/PARAM/tcoin.param
|
123
|
- *Alicia* will double check that this is set the same way in hallc_helicity
|
124
|
analysis
|
125
|
|
126
|
*Richard* needs to add CT vs MM for lambda analysis (log scale CT, no CT cuts)
|
127
|
to confirm whether he sees the same behavior
|
128
|
- we have to deal with the issue either way, but how we approach it would be
|
129
|
different, whether or not he sees it
|
130
|
|
131
|
Dave: Maybe non-Gaussian behavior caused by the reversed signal to CoinTime
|
132
|
module causes it to broaden in the CT spectrum so we're seeing long
|
133
|
non-Gaussian tails
|
134
|
- Dave suggests: Check Heep 10p6, since no randoms shouldn't be seen for clean
|
135
|
elastics. This would allow us to estimate the size of non-Gaussian tails
|
136
|
|
137
|
This suggests two possible ways to correct for the issue:
|
138
|
- Dave's way: use Heep CoinTime distribution to estimate size of Non-Gaussian
|
139
|
CT tails
|
140
|
- Garth's way: subtract "far randoms" from "close randoms" in physics data to
|
141
|
get size of Non-Gaussian tails
|
142
|
- best to check both methods. If consistent within errors, then can apply
|
143
|
easier-to-determine Heep correction to 10.6GeV KaonLT physics data
|
144
|
|
145
|
Richard finds a Heep-COIN 10p6 replay that we can look at
|
146
|
- CT looks very asymmetric even here, non-Gaussian tails -25 -> -5 and +5 ->
|
147
|
+20 ns (plot posted on RedMine)
|
148
|
- heep_coin_time_10p6.pdf
|
149
|
- Cuts applied:
|
150
|
tv__tree->Draw("CTime_epCoinTime_ROC1","abs(CTime_epCoinTime_ROC1)<50 &&
|
151
|
abs(hsdelta)<8 && H_cer_npeSum>2 && ssdelta>-10 && ssdelta<20 &&
|
152
|
P_aero_npeSum<2","", 86385, 0);
|
153
|
|
154
|
Dave: Beta cut may be hiding the issue, a comparison may be useful
|
155
|
- Plot of P_gtr_beta vs CoinTime for Heep-COIN replay
|
156
|
- ctime_vs_beta.pdf
|
157
|
- beta has a bifurcation that occurs outside usual cut abs(beta)<0.3
|
158
|
- Richard and Stephen saw this effect with beta much earlier, but didn't
|
159
|
investigate further
|
160
|
- Alicia coinfirms that 10.6GeV physics data have the same issue
|
161
|
- cointime_beta_10p6.pdf
|
162
|
- *Alicia* will explore CT vs beta to see if cutting it makes much difference
|
163
|
- seems likely that we should remove beta cut as it complicates the
|
164
|
correction for non-Gaussian tails, particularly since beta provides limited
|
165
|
PID information at high momentum
|
166
|
|
167
|
- Alicia and Richard will ask Stephen about this, but this CT asymmetric
|
168
|
peak generally might be a good thing to bring up for the next Quarterly
|
169
|
Analysis meeting
|
170
|
|
171
|
Homework:
|
172
|
- Alicia: confirm that tcoin.param cuts are applied correctly
|
173
|
- Alicia: explore CT vs beta to see if cutting it makes much difference
|
174
|
|
175
|
- Richard: confirm that get same behavior of CT vs MM (although Heep-Coin seems
|
176
|
already to show this)
|
177
|
- Richard: compute Non-Gaussian correction both ways, and we will have to
|
178
|
decide which method is more reliable to apply to data
|
179
|
|
180
|
GH checks logbook, and thinks the CT timing error was fixed by Brad on
|
181
|
2018-Nov-15
|
182
|
- https://logbooks.jlab.org/entry/3626796
|
183
|
- https://logbooks.jlab.org/entry/3626194
|
184
|
- This is during the SIDIS-CSV run between the 10.6 and 3.8 GeV KaonLT data
|
185
|
taking
|
186
|
|
187
|
|
188
|
Next Meeting
|
189
|
------------
|
190
|
- Tues Oct 10 @ 15:00 Eastern/13:00 Regina/12:00 Pacific
|
191
|
- PionLT will go first
|
192
|
|
193
|
Join Zoom Meeting
|
194
|
https://uregina-ca.zoom.us/j/94470211297?pwd=djBROEdWUENLUTF3ZFN1c0kvS0VIQT09
|
195
|
|
196
|
Meeting ID: 944 7021 1297
|
197
|
Passcode: 320362
|