CALICE Tungsten HCAL Prototype status Erika Garutti Wolfgang Klempt Erik van der Kraaij CERN LCD International Workshop on Linear Colliders 2010, October.

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Presentation transcript:

CALICE Tungsten HCAL Prototype status Erika Garutti Wolfgang Klempt Erik van der Kraaij CERN LCD International Workshop on Linear Colliders 2010, October 21

WHCAL experimental setup IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD2 CALICE hadronic calorimeter installed at CERN with: 30 plates of 1 cm thick tungsten as absorber 3x3 cm scintillator tiles as active material with SiPM for readout Alternative detector technologies will join in parallel with the normal data taking Now being commissioned in a muon beam and will move in November to the T9 testbeam line at the CERN-PS (1-10 GeV). Goal of the test: Prove the technology of using tungsten as absorber in an HCAL Validate hadronic shower simulations

Installation in PS - T7 area WHCAL muons 1-10 GeV IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD 3 Three PCs for: - DAQ - Analysis - Power control Muon flux originating from pions in a PS beamline ~30m away - muon beam size ~1m - Energy 1-10 GeV Two 50x50 cm 2 muon triggers installed

Beam instrumentation 2 sets of trigger coincidences: –10x10 cm 2 –50x50 cm 2 (one in front, one behind stack. Not on picture) 2 delay wire chambers commissioned. 3 rd has now also been installed. IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD Two delay wire chambers 10x10 4

Beam instrumentation One set of 8x1 cm 2 to be used for finer measurements For now not in line with beam, but can easily be moved IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD 8x1 cm 2 5

Delay wire chamber commissioning The wire chambers have a delay line running back & forth from left to right, and a line running back & forth from up to down. The chamber gives four signals: time delay from the left, right, up and down sides. IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD LEFT-RIGHT (one chamber) Tested correlation in time of hits from the left and right signal: As a particle hit is read out both sides, then the sum of the two distances (and hence times if the velocity is linear) should be a constant.  Chambers are working correctly 6

Delay wire chamber commissioning IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD7 Arrival time for multiple hits on one channel Red: 1 st Blue: 2 nd Black: 3 rd Left channel Right channel Down channel Up channel Time difference between 1 st and 2 nd hit [ns] Calibration has been performed to convert the time signal to position measurements. Reconstructing of tracks made difficult by multiple hits. Time difference between 1 st and 2 nd hit peaks at 200 ns; most probably reflection.  Will keep the time windows small to minimize #double hits on one channel  3 rd wire chamber is being installed & commissioned at the moment. This will reduce combinatorics.

Muon spills come in ~300 ms window, every 45 sec. Relative timing measured and adjusted where needed for triggers and wire chambers. Using scintillator triggers: –Coincidence of the two 10x10 cm 2 results in ~350 counts/spill –Coincidence of the two 50x50 cm 2 results in ~1000 counts/spill DAQ Rate: 8 Hz (1 ms deadtime / event) Triggering and event rate IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD Spill signal Muon counter 8

Calorimeter commissioning Installation done 30 Aug. – 3 Sept. Noise level consistent with previous installations in testbeams at CERN (2006/2007) and FNAL (2008) Large number of dead channels in modules 24/29/30. (definitions: module = active layer, channel = 1 scintillator tile with SiPM) Not yet clear why, the channels sometimes recover. These channels were known from last FNAL runs to be malfunctioning Yet during pre-assembly at DESY the last few months they showed no problems.  Plans for repair at CERN before November testbeam IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD 9

Calibration & monitoring system SiPM response depends on temperature and voltage  Temperature sensors  LED monitoring system One LED illuminates 18 SiPMs and one PIN to monitor the LED signal. Functionalities of the LED system: –Gain calibration (see later) –Provide full dynamic range for checking the SiPM response function IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD10  LED system tested and operational, except for one module (#20). This CMB has been removed for repair. CMB: Calibration and Monitoring board T: Temperature sensor

Muon events recorded IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD11 In 14 runs collected ~2 million events: calib. & physics physics events events having a track with at least 8 hits in a row (~60%) Not all muons come in perpendicular Will need to take angle into account in calibrations

Trigger delay scan IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD 12 GREEN distribution is results from previous testbeam. RED and BLUE are two runs taken this month with the two trigger setups  Delay (induced by trigger setup) is similar for all modules. The signal from the SiPM is readout after amplifier & shaper, at its maximum value.  Need to determine the delay values (‘hold value’) This has been done already at previous testbeams. –Compared with those results the delay values for all modules should differ by the same amount: Module number Time [x6.25 ns]

calibrated # channels / total # channels: Gain calibration Measured amplitude is converted to digital counts: #ADC gain = #ADC per pixel Gain calibration procedure: use the LED system and take spectra at low intensity light for all channels fit single photon spectra Gain is difference between 2 single photon peak  Gain values extracted and consistent with previous testbeam  Extraction efficiency in last runs at 95%, almost the level it was for previous testbeam. IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD13 efficiency Run number (module 20 excl.) error in data acquisition #ADC counts

MIP energy calibration Selecting straight tracks, and applying calibration from 2007, a single channel results in  Each entry is the energy deposited, expressed in MIP energy as defined in 2007 –Small noise distribution –Fit convolution of a Landau and a Gauss distribution: A MIP = ± mip IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD14 muons noise Extracting this average for each channel results in   Calibration from 2007 looks reasonable  Temperature corrections not yet applied to data Conversion from signal to energy takes more steps than shown – see talk by Zalesak later.

Summary Calorimeter installed and operational –LED system operational (apart from 1 CMB) –Repair of 3 modules will be done before moving to T9 Wire chambers are commissioned Trigger system timed, DAQ rate ~8Hz. Data transfer, conversion & analysis in progress –First results consistent with previous testbeam results –Gain calibration extraction efficiency at 95%  Beginning of November the entire setup will be lifted to the other side of the hall to be placed in PS testbeam. IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD 15

Backup IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD16

Saturation scans One module (1 m 2 ) consists of 216 scintillator tiles of different sizes, with for each tile one SiPM measuring the light. SiPM signal is the sum of signals from fired pixels. –With limited number of pixels and recovery time ( ns) this result in a non-linear response curve IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD17 To extract this response curve, each SiPM is illuminated with increasing intensity  Spread in #ADC saturation approximately factor 2 As expected from the large variety of SiPM #ADC counts LED Voltage [DAC bin] Two dead channels

W-AHCAL will “fly” to T9 on the 3rd of November After commissioning, official CALICE testbeam starts on the 6th of Nov. PS Schedule IWLC - October 21, 2010 Erik van der Kraaij, CERN LCD W-AHCAL move to T9 possible repair 18