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ECAL DPG. P. Meridiani CMS Italia 13/02/2007. Outline. ECAL Achievements in the 2006 Task list & organization of the new ECAL DPG. Achievements in the 2006. From June 2006 ECAL community has been splitted into several experimental setups TB @ H4 (ECAL) TB @ H2 (ECAL + HCAL) Cosmic setup - PowerPoint PPT Presentation
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Paolo Meridiani - INFN Roma1 1
ECAL DPGECAL DPG
P. Meridiani
CMS Italia
13/02/2007
Paolo Meridiani - INFN Roma1 2
OutlineOutline
ECAL Achievements in the 2006Task list & organization of the new
ECAL DPG
Paolo Meridiani - INFN Roma1 3
Achievements in the 2006Achievements in the 2006
From June 2006 ECAL community has been splitted into several experimental setups
TB @ H4 (ECAL) TB @ H2 (ECAL + HCAL) Cosmic setup MTCC
Several achievements in different technical areas Full transition to CMSSW:
• LocalReco • Simulation • DB • DQM
DAQ & Trigger firstly integrated and validated Laser operations towards final setup
Italian contributions has/will been/be flagged
P. Meridiani, A. Ghezzi
F. Cossutti, C. Rovelli
F. Cavallari, S. Rahatlou
G. Della Ricca, F. Cossutti, B. Gobbo, A. Ghezzi
Paolo Meridiani - INFN Roma1 4
H4H4
4 periods, from July 24th to Nov 12th, for a total of ~70 days of data taking, 6300 runs, ~ 2 billions electrons
To summarize: First goal:Intercalibration (9 SM (1 twice), 1/4 of EB)) Energy Scan & linearity (15-250 GeV, in M1, M3, M4 and as function
of eta) Gap & cracks, corners & edges Xtals Monitoring and Laser operation Irradiation (5 Xtals) Trigger primitives Zero suppressions Synchronous running Muons
Paolo Meridiani - INFN Roma1 5
Intercalibration at H4 [1]Intercalibration at H4 [1] 9 SM put on the beam, of which one repeated twice
Better than what expected considering that beam arrived with 1 month delay
At regime intercalibrating 1 SM (1700 xtals) took less than 2 days Different intercalibration methods tested: intercalibration using the
single crystal response
Intercalibration reproducibilityin a two months period (SM22)
5x5 resolution at 0.7% @ 120 GeV
Corrected single crystal response
All 9 SMs
A. Benaglia, P.Govoni, A. Martelli, M. Paganoni, D. Riparo, R. Salerno, V. Tancini
Paolo Meridiani - INFN Roma1 6
Intercalibration at H4 [2]Intercalibration at H4 [2]
In situ intercalibration methods: based on the energy reconstructed in a cluster (typically 5x5)
Different techniques can be used to evaluate single crystal intercalibration (matrix inversion, iterative algorithms)
Performances compatible w.r.t. single crystal intercalibration
A. Benaglia, P.Govoni, A. Martelli, M. Paganoni, D. Riparo, R. Salerno, V. Tancini
Paolo Meridiani - INFN Roma1 7
Energy/position resolution, noise
Energy/position resolution, noise
Analysis is still on going Basically a confirmation of the 2004 results, where most of
the details of the amplitude reconstruction were understood Noise in ADC countsEnergy resolution in 3x3 using 3+5 weights
Preliminary
Preliminary
C. Rovelli
Paolo Meridiani - INFN Roma1 8
More effort has been put on MC validation/tuning/comparison w.r.t 2004. Last possibility to tune MC before CMS
In particular Lateral containment
On going work together with G4 developers to understand/correct discrepancies
Tuning the MCTuning the MC
Using both G4.7 & G4.8 shower is 1% broader in sim (looking at E1/E25) Situation is reversed w.r.t G4.5 (1% narrower sim), change seems to be due to variation in the implementation of multiple scatteringRelative variation with and are instead very well reproduced
F. Cossutti, C. Rovelli, P. Meridiani
Paolo Meridiani - INFN Roma1 9
Dead channel correctionDead channel correction H4 data can also be used to evaluate dead channel corrections Main idea is to measure in the data the correlation between the energy
content of the non-functioning channel with the channels in a 5x5 crystal matrix: Correlation functions depend on the , of the crystal,particle’s energy and impact position
Simple approach and more refined (neural net) have been explored. Both seem to work fine
Energy (GeV)S25re
co_c
orr
/S25re
co
Resolu
tion
(%
)Corrections being implemented as a standard CMSSW moduleAlso map of noisy/dead channels being implemented in Offline DB
Paolo Meridiani - INFN Roma1 10
25ns bunch structure25ns bunch structure
A 25-ns bunched beam was delivered for 10 days (end of september) to H4:
Accelerator clock and orbit signals received by a LHCrx module and distributed to CCS/DCC/TCC via the TTCci.
Trigger Primitives acquired and TCC data written in the event. Used to validate CMSSW TPG emulator
The 25 ns beam sub-structure as seen from H4 TDC.
Paolo Meridiani - INFN Roma1 11
H2H2
Lots of data with different beams (e, - , - on target) with E (1300GeV)More difficult experimental condition environment with respect to H4For example ECAL temperature is not as stable as H4
Also beam contamination: delicate beam cleaning/particleId required for all analysis
Paolo Meridiani - INFN Roma1 12
ECAL intercalibration @ H2ECAL intercalibration @ H2
Intercalibration methods used at H4 have been adapted for H2 running
Temperature variations (±0.1C) (corrections needs to be applied before calibration)
Less statistics for each xtal than H4 Wider beam Beam contamination
S1 calibration results
After cal.
Before cal.
ADC counts
5x5 resolution @ 50 GeV ~ 2% Still larger than expected.
D. Del Re, R. Paramatti, S. Rahatlou
Paolo Meridiani - INFN Roma1 13
Combining ECAL+HCALCombining ECAL+HCAL
On going work: optimization of the combined ECAL+HCAL response
Choosing optimal weights for combining ECAL + HCAL energies
• E=EECAL+EHCAL
Different calibration schemas are being tried in order to optimize resolution and linearity
Paolo Meridiani - INFN Roma1 14
0 run @ H20 run @ H2
20GeV beam
0 0
Runs taken at 3 energies:9, 20, 50 GeV
Being used to optimize the pi0 reconstruction/selection
A simple test of the 0
calibration algorithm has been performed
Before calibration After calibration
Resolution using S1 calibration:(0) ~ 4.8%(0) ~ 3.7%
D. Del Re, D. Franci, S. Rahatlou
Paolo Meridiani - INFN Roma1 15
Cosmic IntercalibrationCosmic Intercalibration
Every integrated SM is/will be tested for around one week using a specific cosmic setup (located in H4)
10° inclined SM APD HV raised to have gain 200 About 5 million triggers are collected for each
SM
Useful for two main reasons Initial commissioning of the integrated SM Preliminary intercalibration coefficient can be
computed at a precision of around 2% for all channels
Systematics w.r.t to beam intercalibration are under detailed study
F. Ferri, A. Ghezzi, S. Ragazzi, T. Tabarelli
Paolo Meridiani - INFN Roma1 16
ECAL @ MTCCECAL @ MTCC
2 SMs at 11 o’clock Gain 200 (S/B 30 for aligned muons) Events with muon signal in ECAL
0.5% of DT trigger 0.15% of CSC trigger
Checks with/without magnetic field Pedestals/Noise
• Observed variation of the value of the pedestal but noise is unchanged
Muon signal amplitude/timing• Amplitude unaffected, small variation of the timing (3ns) still under investigation
Paolo Meridiani - INFN Roma1 17
DAQ & TriggerDAQ & Trigger
ECAL DAQ software system: The ECAL DAQ software system has been used in H4, H2 (HCAL+ECAL)
and MTCC (integrated with Global DAQ & Trigger) Final H4 test-beam version (release ECAL_0_1_0, based on XDAQ_V3.5.2
and SLC3) has been closed and archived. Work to port it to XDAQ_V3.7.3, SLC4 /64-bits is in progress.
In H4 also full DAQ Hardware integration has been achieved Full ECAL triplet: CCS, DCC, TCC MATACQ board: 1-ns sampling of laser pulse for monitoring purpose
TODO: Move toward SLC4 / 64-bits Software system is done to support 36 SMs in EB. To be adapted to
include Endcaps DAQ and Trigger configuration from DB (tables implemented, but read
now from XML)
Paolo Meridiani - INFN Roma1 18
DatabasesDatabases
The DB and its access tools have been operated at H4 and H2 test-beams
DCS Configuration DB (via PVSS) has been tested and works fine. DCS Condition DB (via PVSS) has performance issues. DAQ/Trigger Condition DB: run records and DAQ/Trigger
configuration keys are written in the Condition DB. Writing of summary histograms will be implemented.
DQM (Data Quality Monitor) logging to Condition DB works well. DCU measurements (APD temperatures+currents, electronics
temperatures, LV settings) are written to Condition DB via C++ API.
Most offline DB objects have been implemented and integrated into the CMSSW reconstruction
F. Cavallari
Paolo Meridiani - INFN Roma1 19
DQMDQM
ECAL DQM has been widely used in all the setups 2006 has been spent in continuous update/development/upgrade Many useful low level detector tasks have been implemented, used to
spot problems/debug the system• data integrity• pedestal mean/noise• signal pulse shape• laser/test-pulse amplitude & timing response• trigger primitives activity
Some TB physics oriented task have been also developed• Cosmics occupancy and energy spectrum• beam energy deposit (max crystal, 3x3 matrix)• beam profiles as measured by hodoscope• energy deposit vs. beam position
To be moved towards the CMS physics
F. Cossutti, G. Della Ricca, A. Ghezzi , B. Gobbo
Paolo Meridiani - INFN Roma1 20
An example of a H4 DQM page An example of a H4 DQM page
F. Cossutti, G. Della Ricca, A. Ghezzi , B. Gobbo
Paolo Meridiani - INFN Roma1 21
Laser monitoringLaser monitoring
Laser: needed to track xtal trasparency changes. ~1300 Laser runs taken in the H4 setup.
This data volume is equivalent to 10 hours of full CMS running
All data at H4/H2 have been processed ‘quasi-online’ using the DQM infrastructure. However, this is different from the online “laser farm” that we’ll need in CMS
Stability : APD/PN ratios for each channel
Overall stability good, even without refined corrections. But detailed workflow from laser events to corrections is
still to be demonstrated...
Paolo Meridiani - INFN Roma1 22
Laser MonitoringLaser Monitoring H4 stability
H2: In H2 night/day effects are larger (no room with stabilized T). Anti-correlation between T and APD/PN (~ -2%/°C) as expected.
APD/PN
Stability 1.4 ‰ from gauss fit to peak.
Long tail under study, but overall
stability is satisfactory
H2 testbeam:
Black : APD/PN, averaged over 100 channels.
Red : T/20+1
Paolo Meridiani - INFN Roma1 23
ECAL in-situ calibration: statusECAL in-situ calibration: status
Different calibration methods as described in PTDR needs to be merged into a coherent plan
Since PTDR: big effort has been put on 0 calibration 4 internal notes have been produced by different groups To exploit full potential these events need to be selected
from L1 accepted events Special stream/trigger techniques are being designed
Additional effort: improve/put calibration in CMSSW. 2007 should be dedicated to
Coherent plan for calibration including first year data taking Definition of detailed workflow
D. Del Re, D. Franci, P. Govoni, M. Paganoni, A. Palma, R. Paramatti, S. Rahatlou, R. Salerno
Paolo Meridiani - INFN Roma1 24
TasksTasks
DQM Coordination and responsible for basic services Many of the other tasks listed below involve or require DQM
Amplitude reconstruction And digitization
DCC operation Data unpacking, and Digi to Raw translator; endcap specific mapping
issues
TCC operation Trigger Primitives
Emulation
Selective Readout Processor Emulation; algorithm(s) for low luminosity
Synchronization and timing
Paolo Meridiani - INFN Roma1 25
Tasks[2]Tasks[2] Databases Calibration and alignment
Calibration methods and algorithms• Use of “precalibration”• Phi symmetry 0 • Z→ee• Z→• Single electron
“low level calibration”• Pedestals; gain ratios; dead channels
Crystal transparency corrections (Laser) Alignment
Clustering And cluster corrections
Simulation Geometry (new into CMSSW 140) Shower simulation
Paolo Meridiani - INFN Roma1 26
Tasks [3]Tasks [3]
Preshower issues Try to integrate the preshower aspects within the other categories
Event display Global performance monitoring
alias offline DQM
Paolo Meridiani - INFN Roma1 27
Sub-boxologySub-boxology ECAL framework
Data format, raw data, time frames,amplitude reconstruction, application of calibration constants
Reconstruction Clustering, superclustering and corrections
Calibration and alignment Calibration Laser transparency corrections Alignment Low level calibration (pedestals, gain ratios…) ?
Simulation Geometry Shower simulation (GEANT and FAMOS)
Databases DQM Testbeam analysis
Paolo Meridiani - INFN Roma1 28
ContactsContacts Offline: Reconstruction
Low level reconstruction: Paolo Meridiani (ad interim) Clustering: David Futyan (ad interim)
Offline: Simulation Overall: Fabio Cossutti (ad interim) Geometry: Brian Heltsey
Offline: Level-1 trigger Trigger primitives: S. Baffioni
Offline/Commissioning: calibration and alignement Overall: to be defined Alignment: Brian Heltsey Transparency correction (laser): to defined
Offline: Analysis tools Requested…
Physics: JetMet Requested…
Paolo Meridiani - INFN Roma1 29
ConclusionsConclusions
2006 has been a fundamental year for the ECAL project 10 SM have been intercalibrated with the beam All integrated SM undergo to cosmic calibration DAQ + DQM integrated and tested in different setups First validation of CMSSW Offline software + DB achieved
2007: solid base to start from but refinement/completion work is
needed in many areas Primary goals
• Prepare everything for commissioning • Deliver a full coherent picture for calibration/corrections
Italian community plays an important role inside ECAL DPG covering many aspects/tasks