Project

General

Profile

Kaon LT Meetings » mtg_22dec07.txt

Garth Huber, 12/07/2022 11:56 AM

 
1
                 Dec 7/22 PionLT/KaonLT Analysis Meeting Notes
2
                 ---------------------------------------------
3
                           (Notes by GH and SJDK)
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, Stephen Kay, Ali Usman, Alicia Postuma, Nathan Heinrich
13
CSULA - Konrad Aniol, Erika Gwin
14
CUA - Richard Trotta
15
JLab - Dave Gaskell
16
Ohio - Julie Roche, Jacob Murphy
17
FIU - Pete Markowitz
18

    
19
Richard Updates
20
---------------
21
- LT separation code
22
   - it's slow getting information back from Bill
23
- Heep analysis
24
   - SIMC/hcana calculate variables differently
25
   - Adding new variables that calculate it in the same way as hcana into SIMC
26
   - DG - In complete recon event or a new subroutine?
27
      - In a new one
28
      - DG - Should be fine
29
         - Maybe call it "recon_hcana"?
30
         - Don't do it as a separate branch!
31
            - Will be annoying to integrate, also everyone will want this
32
         - New submodule is good, will be modular then
33
- Total Efficiencies per run for each setting
34
   - Needed input into Bill's LT-sep code
35
      - Haven't incorporated Ali's updated efficiencies
36
         - Error bars are off as a consequence
37
         - Some are grabbing the wrong calculations too
38
   - -t binning plots/demonstrations shown for Runs 4965-5009 Left-Cent-Right
39
      - ~2% downtrend seen in Effs for Right setting, probably following real
40
        changes in running conditions
41
      - Actual t-binning and diamond cuts will be done in Bill's LT-sep code
42
      - Need to use Jacob's code to apply diamond cuts
43
   - GH - For MMK plot, should zoom in on Lambda peak and see if it's
44
     stable versus run number. Apply finer binning too
45
      - RT - Will add it, will do 2D phi dist too
46
   - GH - also need to add a slide of what Effs and typical values are used in
47
     the TotEff calc, so we can see exactly what was done
48
     
49
   - *Need to do a HMS calorimeter efficiency study*, can't rely on what
50
     the report file gives
51
      - DG: this needs to be for all PID detectors
52
      - need to select some runs which are sufficiently clean and then apply
53
        the obtained values globally, preferably vs. spectrometer momentum
54
	 - often, can never get rid of enough pi- (for HMS), so might even
55
           have to resport to Heep data, but then have to worry about not
56
           illuminating the full focal plane
57
      - the studies are simple, but this needs to be completed before starting
58
        LT-separations
59
     
60
- iFarm issues
61
   - Tape silo had a robotics failure yesterday, can't get stuff from the tape
62
     silo currently
63
   - can only replay data already cached to disk
64

    
65
Ali Updates
66
-----------
67
- Updates to Error Calculations
68
   - Heep coin data from 6.2/8.2/10.6 GeV
69
   - Error bars were too big
70
   - New calculation using binomial errors
71
   - need to *add* a slide showing old and new calculations
72
   - New calculation shrinks error bars quite drastically
73
   - For 8.2 Gev, maybe even too small
74
   - 10.6 GeV looks good with one outlier
75
      - All efficiencies seem to be lower for this point
76
      - Has lowest beam on time?
77

    
78
- DG - Need to *correct* EDTM LT for time the beam is off
79
   - the issue is that the EDTM keeps counting when beam off, need to
80
     correct the scalers via an approximate formula derived by PBosted
81
   - Richard's Lumi script should do this?
82
   - DG - *Current off correction* from PBosted study:
83
      - LiveTime=(Rmeas-(1-f))/f
84
      - Rmeas = edtm_accepted/edtm(nominal edtm live time)
85
      - f = current(no cut)/current(with threshold)
86
      - this formula is an *approximation*, assumes the beam ramp up time is
87
        negligible, which may or may not be true, depending on the running
88
        conditions, probably this approximation will be worse for early 10.6
89
        GeV running
90
    - AU - probably tnis is NOT implemented yet for Heep, physics settings,
91
      will discuss with RT
92
   
93
- Delta-Pi
94
   - Ali has received an invitation from Stefan Diehl to present some Delta-Pi
95
     results at a conference at ECT* in Trento in August
96
   - will discuss JLab conference travel funds application with RT 
97
 
98
Stephen Updates
99
---------------
100
- No new progress on RF class
101
   - Will update hcana in group directory to use new RFtime variables
102
   - Stephen will try to do this today, let him know if there are any issues
103
     with the new hcana version, should only affect the CT/RF classes
104
   - Should not need a DEF file change
105
      - RFTime.* is in there currently, this will pick up new variables
106

    
107
Alicia Updates
108
--------------
109
- BSA analysis
110
   - Edited report files to calculate effs separately for each helicity
111
   - Can't separate charge by helicity
112
      - Will cut charge in half to normalise dummy subtraction
113
   - DG - Should contact Steve Wood wrt to helicity scalers
114
      - Might've been added for A1n/d2n?
115
      - SK - Would explain why helicity scalers didn't work for KaonLT but were
116
        added later (but still had issues)
117
      - AP Should CC Carlos Yero when asking Steve on this
118
   - shown runs have same TotEffs for +,- helicity to 3rd decimal point
119
     but LH2, Dummy do have a different Effs
120
      - DG - HGC pion efficiencies are way too low
121
      - Just set them to 1 until RT/AU complete their study
122

    
123
   - Weighted average of BSA for Left-Cent-Right
124
   - Experimented w/Complete fit (A=sin-phi,B=cos-phi,C=cos-2phi) and
125
     Approximated fit (A=sin-phi only)
126
      - complete fit is over-fitting the data, ending up with B,C>A for some
127
        fits
128
      - DG - can constrain B,C based on world data
129
         - we have LT,TT from Fpi-2 but only up to Q2=2.45
130
	 - also have CLAS data
131
      - SK - Glancing back at old code from his PhD analysis @ Mainz:
132
       he ran an *initial fit* with just one Sin/Cos term (dashed red for
133
       Alicia), and then fed this into the second fit
134
         - Can adjust the second fit in a few ways then, can constraint the
135
           asymmetry A to vary in some range, such as permitting A to only vary
136
           within 1-2sigma of initial fit
137
         - B/C can also be restricted too
138
      - Julie discusses some of the difficulties of interpreting the results
139
        that were used when presenting DVCS BSA data
140
         - Suppressing B,C terms can make things look "more precise", but
141
           actually shrinks the error bars in an unrealistic manner
142
	 - in the end, the DVCS paper presented both sets of results in a paper
143
           and gave a caution that the result and obtained error bar depends on
144
           how the analysis is done
145
         - GH - Could quote weighted everage of complete/approx fits?
146
	 
147
   - DG - What about *radiative corrections* to the BSA?  This is an issue that
148
     just occurred to me now
149
   - GH - Unlike the LT-sep results, we aren't quoting a cross section. Not
150
     using SIMC to get asymmetry, while we use SIMC in the ratio method to
151
     get the cross sections
152
      - DG - Yes, Acceptances should cancel in the BSA
153
   - GH - From SIMC studies for LT data, can *estimate* how large radiative
154
     corrections are for a t bin by turning on/off the rad-corr in SIMC and and
155
     how large the effect is, no easy way to see how this corrects the
156
     asymmetry
157
   - DG - Iterative fit? Put SSA into SIMC and see how it changes things when
158
     RadCorr On/OFF
159
        - maybe can also use SIMC to do t-bin centering for BSA, just like we
160
          do for the cross sections via the Ratio Method
161
   - DG - Interesting question, could be an advantage over CLAS analysis in
162
     that we can actually study and estimate the RadCorr effects.  Will think
163
     about this further
164

    
165
Next Meeting
166
------------
167
Wed Dec 14 @ 9:00 Eastern/8:00 Regina/6:00 Pacific
168
- PionLT will go first
169

    
(142-142/559)