Project

General

Profile

Kaon LT Meetings » mtg_23nov16.txt

Garth Huber, 11/17/2023 12:39 PM

 
1
                 Nov 16/23 PionLT/KaonLT Analysis Meeting Notes
2
                 ----------------------------------------------
3
                            (Notes by GH & AH)
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
CUA - Richard Trotta, Tanja Horn, Casey Morean
15
JLab - Dave Gaskell
16
CSULA - Konrad Aniol
17

    
18
Richard
19
-------
20
Optimization of offsets for high beam energy datasets
21
- new study based off GH's older 5_recon offsets, adjusting dPe offset, keeping
22
  dPp=-0.1%
23
 - dPe has a greater effect on W
24

    
25
- then try GH's new offsets, determined with dPp constrained
26
  - these work fairly well, but RT adjusts dPe to optimize W, EM overlap
27
  - Displayed different variables after including offsets. It seems that some
28
    variables get better with some extra variation.
29

    
30
- Garth: concerned about optimizing offsets for Heep, which may not work for
31
  other data.  Better to determine global offsets, for multiple beam energies,
32
  so we have some confidence they can be applied to physics data.
33
  - RT will try to get 3 sets of offsets:
34
    a) 3.8, 4.9, 6.2 GeV
35
    b) 8.2 GeV, where the SHMS - HMS spectrometer roles are reversed
36
       - fortunately, the SHMS, HMS momentum offsets are similar
37
    c) 10.6 GeV, where there may be HMS saturation
38

    
39
- Dave: are the optics fine for HMS=6.6 GeV/c setting @ 10.6 GeV?
40
  - yes, using Jacob's Matrix Elements, sieve spots look okay
41

    
42
  - RT is actually using smaller offsets than GH provided for energies other
43
    than 10.6
44

    
45
Ali
46
---
47
Coin Time vs. Beta leakage in 10.6 GeV data
48
- completed the cut-dependence study requested by Tanja/Dave
49
  - ~96% efficiency @ 10.6 GeV, >99% for 6.2, 8.2 GeV
50

    
51
- Mark sent a write-up on Improved Hodoscope timing and Hit reconstruction
52
  algorithm
53
  - initial test of ptof_tolerance from 100ns to 2.0ns had no effect
54
    - the problem was traced to AU adjusting the wrong cut file
55
    - a set of dedicated cut files were used for certain sets of run #
56
  - now the smaller tolerance works, the cointime vs beta tails gone, no events
57
    lost
58

    
59
- the problem seems coming from too loose time window on the hodoscope, our
60
  earlier hypothesis that it was related to inverted signal cable was a red
61
  herring
62

    
63
  - Nacer: what is the meaning of this tolerance?
64
    RG/Casey: times from all hodoscope hits are propagated to the focal plane,
65
    ptof_tolerance is the time window to accept different hits from the
66
    hodoscopes when reconstructing an event
67
  - 100 ns clearly far too loose, 2ns (a beam bunch spacing) should be good
68
    since TOF variations to the hodoscope planes is taken into account in the
69
    focal plane projection
70

    
71
  - fortunately, the ptof_tolerance was already set correctly for the 6.2, 8.2
72
    data, it's a mystery that only the 10.6 GeV data had such a wide window
73
    - Garth: we've had repeated issues with things set wrongly in the 10.6 GeV
74
      replay.  Really hope we have caught them all now.
75

    
76
  - Ali will update the cut files and make a pull request.  A full replay will
77
    be submitted after RT has finalized the offsets.
78

    
79
Vijay
80
---
81
OOP offsets
82
- applied 0.99 mrad HMS offset, obtained from GH's fit to just 2.7,3.6,4.6 GeV
83
  data
84
- PMY variable is improved for all 3 beam energies
85

    
86
- Dave: investigated change in beam angle in different beam periods.  The
87
  changes were of order ~0.1 mrad, not 1 mrad, so not enough to explain why we
88
  need different OOP offsets for different beam periods
89

    
90
Alicia
91
------
92
No report, was looking into CoinTime issue reported by Ali, and corresponded
93
w/M.Jones
94
- will do a 10.6 GeV pion replay (including helicity info) after RT has
95
  finalized offsets
96

    
97
Nacer
98
-----
99
Checking 3.8 GeV hodoscope calibrations after finding shifted beta distribution
100

    
101
Nathan
102
------
103
CoinTime reference times
104
- Checked multiple T.coin.pTRIG.ROC variables, and looked at different
105
  multiplicity cuts
106
  - Plot of T.coin.pTRIG1_ROC1_tdcTimeRaw
107
    Blue: No cuts, Red: MULTIPLICITY=1
108
- MarkJ indicated need to separate SINGLES and COIN events, to avoid multiple
109
  peaks and allow cut windows to be tightened
110
  - will need separate cuts for SINGLES and COIN, different PTRIG
111
  - For most variables the timing window cuts are clear
112

    
113
- T.coin.pT2_tdcTimeRaw has all events at zero, needs further investigation
114

    
115
Junaid
116
------
117
- Finished hodoscope calibration, changes pushed today
118
  - will post documentation slides on RedMine
119
- Moved to drift chambers calibration. Started with with 2021 data for both HMS
120
  and SHMS
121
  - Drift distances for different drift chamber planes look better before
122
    re-calibration, so it seems the calibration is okay
123
  - submitted 40 more jobs for more thorough check
124

    
125
Next Meeting
126
------------
127
- No meeting next week due to US Thanksgiving
128
- Thur Nov 30 @ 15:00 Eastern/14:00 Regina
129
  - PionLT will go first
(318-318/570)