1convenors meeting, Sep 4th 2003G.B. for CALGO Calorimeter Algorithms A few remarks on the calo....
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Transcript of 1convenors meeting, Sep 4th 2003G.B. for CALGO Calorimeter Algorithms A few remarks on the calo....
1convenors meeting, Sep 4th 2003 G.B. for CALGO
Calorimeter Algorithms
A few remarks on the calo. problems
Overview of the CAT force results
From CAT to CALGO
Results of the CALGO workshop
The road ahead
Gregorio Bernardi for the
CALGO and CAT groups
2convenors meeting, Sep 4th 2003 G.B. for CALGO
DISCLAIMERDifferent more or less important problems affect the calorimeter
However:
The calorimeter data are “waiting” for other subdetector data improvements in order to go to publication:
The Reprocessing is NEEDED mainly to improve the Tracking
The Calorimeter “fixing” can be done and redone and redone from the TMB’s in a few days.
personal opinion: From the analysis point of view the fake jets problem is, for the moment, our main problem in the calorimeter.
3convenors meeting, Sep 4th 2003 G.B. for CALGO
D0 Calorimeter Algorithms Task Force
Members of the Task Force (MAY –JULY 2003)
Gregorio Bernardi (chair), Jonathan Hays, Serban Protopopescu,
Markus Klute, Jan Stark, Robert Zitoun, Vishnu Zutshi
+ Emmanuel Busato, Jean-Roch Vlimant
Charge to the Task Force:
The task force will optimize in collaboration with the Physics and
ID-groups the calorimeter algorithms for precision physics. It will
start from the achievements of the Calorimeter Task Force, continue
to improve the algorithms and propagate them to the physics objects
using as benchmarks the comparison data/simulation of the W (->e nu)
transverse mass spectrum and Jet & Met resolutions in di-jet events.
The task force is expected to coordinate the efforts in the different
groups related to the calorimeter.
4convenors meeting, Sep 4th 2003 G.B. for CALGO
Specifically, the task force should:
1) Make progress on the understanding/correction of the calorimeter noise.
2) Finalize the development of an optimized 0-suppression scheme and study
its consequences for MET, EM, Tau and Jet ID.
3) Make progress on the understanding of the EM response/resolution, using
on-line and off-line tools.
4) Make progress on the data/mc agreement of the calo object
reconstruction and of the energy flow algorithm.
5) Use large statistics of W and di-jets events to display how the
progress achieved on points 1-4 propagates in the corresponding
physics distributions.
5convenors meeting, Sep 4th 2003 G.B. for CALGO
Correcting the DATAMany problems are not discovered immediately online. - BLS electronics problems - cable swaps - not all hot cells are caught online
Large datasets on tape with some quality issues.These data sometimes suffer from isolated problems. Can fix theseisolated problems and use the data for publication quality analyses.But: need mechanisms to do this.
cal_corr_dst packageTakes raw calorimeter data and fixes known problems
included in reprocessingCan also be included in user analysis jobs
(because we have the individual cell energies in the thumbnail).Requires some effort as calorimeter reconstruction needs to be rerun.
CAT MODEL HAS BEEN TAKEN ON BOARD BY COMMON SAMPLE GROUP C. S. group now centrally fixes the TMBs (while we are waiting for the
result of the p14 reprocessing).
6convenors meeting, Sep 4th 2003 G.B. for CALGO
DQ Issues Addressed in Current Version of cal_corr_dst
- Energy sharing problem Draft D0 note: http://www-clued0.fnal.gov/~stark/esp_note.ps
- Tower two problem Draft D0 note: http://www-clued0.fnal.gov/~stark/tower2/note.ps
- BLS cable swap next slide
Short term project:
kill hot cells found by dq_calo
Web page with latest version of cal_corr_dst:
http://www-clued0.fnal.gov/~stark/cal_corr_on_tmb.txt
7convenors meeting, Sep 4th 2003 G.B. for CALGO
Most recent addition to cal_corr_dst
J. GardnerCorrection for BLS cable swap:
The “discovery” of the swap was triggered by an analysis plot
/ distribution of all EM candidates:
pT > 25 GeV EM fraction > 0.9 isolation < 0.15 HMx8 < 20
pink boxes: tower two problem
blue boxes: energy sharing problem
red boxes: don’t know yet…
Nice example of constructive feed-back from analysis.
Donuts ? Cable swaps !
8convenors meeting, Sep 4th 2003 G.B. for CALGO
Reducing influence of Noise: T42
T42: reject ALL isolated cells below 4 sigmas (and ALL negative energy cells)
Select high signal cells (4 sigma)Keep their significant neighbours (2 sigma)
Thresholds 2 is 2.5 at the moment T42.5
What neighbours means
Available in D0Reco in shadow mode
Not running yet:
We wants to have first a tmbfix w/o T42
Full description is available in DØNotes
4124, 4146
9convenors meeting, Sep 4th 2003 G.B. for CALGO
T42 on high energy electronsEstimators for EM candidates in data, when pT>13 GeV
OK !
10convenors meeting, Sep 4th 2003 G.B. for CALGO
T42 on Missing and Scalar ET
WZ skim , p13.06 , W e nu selection (ET > 20 GeV, MET > 25 GeV)
Compared to Pythia MC
No T42
After T42
11convenors meeting, Sep 4th 2003 G.B. for CALGO
Top group’s alljets skim (reco version p13.06.01) : * Passes the 4JT10 trigger.
* At least 4 jets (JCCB). * HT > 100 GeV (just plain sum of uncorrected JCCB
jets). 20000 events
Jets are JES corrected.No quality cuts applied because jet id distributions change significantly.
t42 no t42
Jets properties before and after T42
12convenors meeting, Sep 4th 2003 G.B. for CALGO
Jets not found with new seeding :- mostly low pT - in ICR- large number of proto-jets merging
mean = 0.43mean = 2.22
Jets not found with new seeding:
Jets found in both cases:
about 3-4% less jetswith new seeding
Remove CH and MG cell energies from the seed
tower energy before starting preclustering
(i.e., a p13 seed might have an energy < 500 MeV
in p14)
New Jet Seeding in p14
13convenors meeting, Sep 4th 2003 G.B. for CALGO
JET – ID: Plans for the future
High priority task remains reduction of fake jetsAre T42, new jet seeding, hardware fixes enough ?
Jet ID cuts new certification Use L1 confirmation ?
Tuning of Jet ID criteria for ICD region.
Tuning of merging algorithm ?
Consider lowering jet pt threshold 6 GeV (to make analysis at 10 - 12 GeV)
14convenors meeting, Sep 4th 2003 G.B. for CALGO
MET subgroup Goals
MET Resolution: related to Jes, T42 …
Treatment of non reconstructed jets
Overall correction strategy of MET Decides how to correct EM/Jets etc..
Understanding of unclustered energy - in QCD processes- in EW events
15convenors meeting, Sep 4th 2003 G.B. for CALGO
CALGO: Activities & StructureCALOP - calo hardware & operationsR. Zitoun
cal/icd-softw.Jan Stark/Lee Sawyer
cps-software A. Magerkurth/D.Alton
fps-softwareA. Patwa/A. Turcot
em-id Harald Fox, Jan Stark
tau-idDhiman Chakraborty / Serban Protopopescu
metPatrice Verdier, Sophie Trincaz
jesIa Iashvili/Nirmalya Parua
-id Yurii Maravin Drew Alton
jet-idSlava Kulik Alexander Kupco
l3cal-software
cal-simulationLeslie Groer, Michel Jaffre’
CAT
eflowAnna GoussiouJon Hays
hardware
data taking
slow control
trigger L1/L2
icd
CALGO - calorimeter algorithms & objectsU.Bassler/ G. Bernardi
calib – online
cal – dq Slava Shary,
Jan Stark
16convenors meeting, Sep 4th 2003 G.B. for CALGO
Welcome/Goals of the Workshop (15') U. Bassler/G. Bernardi
Shutdown Status/Operation Organization R. Zitoun
Data Quality V. Shary/J. Stark Overview J. Stark zero-bias monitoring & bad cell correction V. Shary
Level 3 (20') V. Buescher
Simulation Status and Prospects L. Groer
Tau-id D. Chakraborty/S. Protopopescu Jet-id S. Kulik/A. Kupco jet-id status and plans S. Kulik jet reconstruction and simulation V. Zutshi Jet and Met while studying Wbb production G. Bernardi
Missing ET (30') S. Trincaz/P. Verdier MET status (15') P. Verdier cal_t42 status (15') J.R. Vlimant
CALORIMETER WORKSHOP contributions
17convenors meeting, Sep 4th 2003 G.B. for CALGO
Jet Energy Scale I. Iashvili/N. Parua
JES status and plans I.Iashili
Response measurement for b-jets T.Kurca
Showering measurement with MC method J.Rani
Energy Flow (30') A. Goussiou/J. Hays
electron-id/calibration H. Fox/J. Stark
Introduction H. Fox/J. Stark
EM reconstruction packages S. Crépé-Renaudin
H-matrix, data/MC agreement M. Jaffré/T. Vu Anh
Electron likelihood (2*) J. Kozminski, S.-J. Park
EM scale corrections (10') S. Kermiche
photon-id D. Alton/Y. Maravin
FPS software J. Lazaflores/A.Patwa
CPS Status D. Alton
18convenors meeting, Sep 4th 2003 G.B. for CALGO
Jet Energy Scale Offset (p13.06 data, p13.08 MC)
Response (p13.06 data, p13.08 MC)
New ICR correction (p13.06 data, p13.08 MC)same as previous correction in data (~25%), smaller in MC (11% 6.5%)
Special Min Bias runs Pythia UE + 0.8 minbias
19convenors meeting, Sep 4th 2003 G.B. for CALGO
OffsetLuminosity dependence OK
ResponseIncreased statistics: 15 55 pb-1
EM scale included Systematics: background, topology,
vertexMC used for extrapolation at high
energiesTotal
in central region: 9.5% 5.5%
JES: Smaller Uncertainty
|η|=0.0
20convenors meeting, Sep 4th 2003 G.B. for CALGO
Response: b-jets vs q-jets (MPF method)
T
TmisTjet
E
nER
ˆ1
21convenors meeting, Sep 4th 2003 G.B. for CALGO
Jet Resolutions
Resolution at ET~50 GeVRun I 11.6%Run II 14% (data/MC)
More to Understand !
Z → bb resolutionvarious algorithms (p13.08, uncor.)
Rcone= 0.5 18.1%Rcone= 0.7 17.5%0.4 kT 18.3%1.0 kT 17.7%
Rcone=0.5before correction 18.1%after JES correction 17.0% Use Tracks+clusters?
22convenors meeting, Sep 4th 2003 G.B. for CALGO
JCCA cone jets have no energy correction appliedCellNN calibrated using linear fit to response measured using single charged pion Monte-Carlo.Potential significant improvement: need to calibrate tracks/objects on data. Here results zqq MC with p13
23convenors meeting, Sep 4th 2003 G.B. for CALGO
Electron identificationcalorimeter cells
clusters
electron candidates
electron candidatesfor analysis
The whole chain needs to be certified.
Quite some Monte Carlo dependence: geometric corrections, training of H-matrix, analysis, …
sophisticated discriminants:H-matrix, likelihood
cone, cellNN
C/FPS clusters
trackspossibly with dE/dx
calibration - geometric corrections - EM scale corrections - phi cracks
For low-pT non-isolatedelectrons: road method.
Start from tracks, look atenergy deposits in a narrow road around thetrack extrapolated through the calorimeter; see if thesedeposits are EM-like.
24convenors meeting, Sep 4th 2003 G.B. for CALGO
Low-pT di-EM triggers in trigger list v12.x
7.6 pb-1
Fit result (signal parameters):
N (one tight) = 614 +/- 113
Mass = 3.040 +/- 0.005 = 0.071 +/- 0.005a = 0.61 +/- 0.12n = 1.7 +/- 1.1
Reconstructed using road method.
Trigger list v12 contains a new low pT di-EM trigger. useful data samples for EM validation studies
Summary of the selection criteria used by this trigger:L1: CEM(2,3.) CEM(1,6.) TTK(2,3.) TTK(1,5.)L2: || restriction to central regionL3: two road electrons ( > 3 GeV and > 5 GeV, one tight one loose)
25convenors meeting, Sep 4th 2003 G.B. for CALGO
Data: J/, e+ e- using EM clusters
N (J/Psi) = 152 +/- 15Mass (J/Psi) = 3.166 +/- 0.040 GeVResolution (J/Psi) = 0.382 +/- 0.043 GeV
N (Upsilon) = 70 +/- 18Mass (Upsilon) = 10.31 +/- 0.18 GeVResolution (Ups) = 0.584 +/- 0.144 GeV
Fit results (signal parameters):N (J/Psi) = 82 +/- 9Mass (J/Psi) = 3.166 +/- 0.040 GeVResolution (J/Psi) = 0.305 +/- 0.037 GeV
N (Upsilon) = 55 +/- 13Mass (Upsilon) = 10.12 +/- 0.17 GeVResolution (Ups) = 0.689 +/- 0.190 GeV
HMx8 < 50 HMx8 < 20
comparison of fitted yields gives information on HMx cut efficiency.
26convenors meeting, Sep 4th 2003 G.B. for CALGO
Calibration at low Energy
To investigate the high mass, take theHMx8 < 20 sample and compare the massdistributions obtained from clusters and tracks for the same events. mass obtained from tracks appears to bemore reasonable, but need to check resolutions with Monte Carlo.
mass fromEM clusters
mass fromtracks
yield Mass (GeV) resolution (GeV)
clusters
55 +/ 13 10.12 +/- 0.17 0.69 +/- 0.19
tracks 68 +/- 11 9.43 +/- 0.11 0.62 +/- 0.10
Potential calibration Improvement
27convenors meeting, Sep 4th 2003 G.B. for CALGO
Electron Resolution
From Monte-Carlo with corrections
S = (0.199 ± 0.008)% N = (0.42 ± 0.08) GeV C = (0.0076 ± 0.0014)%
MC momentum resolution 3% @ 50 GeV
expect: Z mass resolution 2%Z MC 2.2%
Data 4.0% 3.1 %
E
NC
E
S
E
28convenors meeting, Sep 4th 2003 G.B. for CALGO
Various Corrections
Corrections in D0reco + emcandidate
Furthercalibrationcorrections
Other trials
MZ/GeV Z/GeV Z/MZ(%)
raw ADC 81.5 3.6 4.4
non linearity 86.7 3.7 4.3
gain correction 86.6 3.6 4.2
crate equalization 86.5 3.6 4.1
geometric correction
90.2 3.6 4.0 ± 0.1
calibration timing 90.2 3.6 4.0
physics timing 90.2 3.6 3.9
calib/phys amplitude
90.0 3.4 3.8
after tuning weights
90.4 3.3 3.7
use 2 calweights 90.4 3.3 3.7
pulser amplitudes 90.2 3.4 3.8
10 slices 90.4 3.3 3.7
29convenors meeting, Sep 4th 2003 G.B. for CALGO
Module Boundaries (Phi) ?
CC has 32 modules with =0.2loss of clusters (?)loss of energy
Broader effect on mass
Cluster no vs track angle
Cluster Evs cluster angle
shower profileout in
MZ/GeV Z/GeV Z/MZ
All 90.4 3.3 3.7
||>0.05 91.3 2.8 3.1
||<0.05 89.6 3.2 3.6
smallest distance to crack→
mas
s
Broader effect on mass
Origin ? Statistics ?
30convenors meeting, Sep 4th 2003 G.B. for CALGO
Dead Material Simulation
Modeling of the phi cracks (electric fields and charge collection)Modeling of the dead-materialModeling of preamp charge collection signal Improvement done for solenoidImproving the material map for the SMT cables, infrastructure, cooling…
31convenors meeting, Sep 4th 2003 G.B. for CALGO
EM ID estimators: data vs MC
p14.03.00 data and MCEM ID v4.12 good electrons, pT > 20 GeV, |
_det| < 2.5, not within cracks, Mee > 50 GeV
At least 1 track match in data
Many distributions are okpT, isolation, transverse shower
shapes in r-phi, EMfractions, HMx41 CC
Discrepancies in a few (MC normally narrower)HMx8 components:#2 (~ logE and z) and #4 (z)Number cells in lower layers CCCC profile/shower shape in and
R HMx6 ?
EM CC Cluster widths in r-phi
EM CC Cluster widths in z
32convenors meeting, Sep 4th 2003 G.B. for CALGO
CPSSpatial resolution Resolution in of 1.58 mr (MC 1.5 mr)Resolution in z of 3.2 mm(MC 2.5 mm)
E/E
MC study: energy resolution Green shows the improvement using the CPS.
33convenors meeting, Sep 4th 2003 G.B. for CALGO
Progress on Photon IDCurrently, a photon is an electron with no matched central track, Why is this not good?
HMatrix does not work well for electrons, not easy to make it work for photons
NEW TOOLS UNDER STUDY:
Tracks Matching tracks to CPS-EM objectsIsolation
Hit countingUse both CFT and SMT
PSMatching to EM/TRKShapes of clusters, separation?
HMxCheck if electron HMx works well enough on photonsTrain it on a sample of
34convenors meeting, Sep 4th 2003 G.B. for CALGO
TRK-CPS-EM matchingFrom a sample of good Zee
candidatesRequire exactly two good EM
objectsMatch them with CPS clusters: 3d floor method:
Match CPS and EM (3d floor) in (, ) space
2 method:Use all floorsFit to a straight line
Wrong clusterGood cluster
d = 0.00683
d = 0.00671
3d floor
3d floor
35convenors meeting, Sep 4th 2003 G.B. for CALGO
Priority Tasks
• Em-energy resolutions (electrons, photons)
• Data/simulation agreement: shower shapes, cracks
• Data quality strategy (on-line/off-line)
• Noise understanding / Fake Jets / T42 integration
• J.E.S. / hadronic energy resolution
• Calorimeter compensation studies (E-Flow)
• -id
36convenors meeting, Sep 4th 2003 G.B. for CALGO
Future dates
CALGO meetings devoted to specific projects:
October 21st: met corrections, DQ October 28th: em-resolution /
simulation …
p14 certification of calorimeter software and objects: November 21st (JES: Nov. 28th)
god-parenting by CAT
Next calorimeter workshop: December 2nd/3rd or 3rd/4th
37convenors meeting, Sep 4th 2003 G.B. for CALGO
Backup slides
38convenors meeting, Sep 4th 2003 G.B. for CALGO
METxy
SET>
rms MET-xy
MET Run Selection
Using METB (no CH, except in good JCCB jets)
Pretty stable with time (METxy most sensitive)
Good run selection based on
rms(METxy)
<SET>
91% good runs (feb-jun 2003) could be lower with tighter cutscould be higher with software
correctionsMUST be update for p14 for TMBfixed data
22 yxxy METMETMET
Only good runs
39convenors meeting, Sep 4th 2003 G.B. for CALGO
TRK-CPS / TRK-CPS-EM matching
Require exactly two CPS-EM objectsPropagate track to the middle of CPS
Calibrate track propagation Check TRK-CPS relative alignment
Select the closest track in (z, ) space
In the Zee sample:TRK-EM (traditional) matching probability is 84 ± 2% (AA)TRK-CPS-EM matching probability is
floor method: 95.8 ± 1.1% 2 method: 92.8 ± 1.3%
Fake rate estimation is in progress
40convenors meeting, Sep 4th 2003 G.B. for CALGO
JES: b-quarks & parton-level
b μν + X
b c μν + X
New semi-leptonic correction for b-jets (p13.08 MC)Added dependence on parent quark (in addition to Emu,
ptrel, Ebjet
Parton-levelCorrection:
light qb-q