ECAL (inter)calibration and monitoring ECAL è un rivelatore bellissimo ma non esattamente facile per farlo funzionare. La difficoltà aumenta tanto più il calorimetro è preciso, ogni cosa diventa importante per raggiungere la precisione voluta. ECAL ha tanti fisici quanti DT, RPC e CSC sommati (ma siamo la meta’ del TRK…), circa 30 persone lavorano in ‘calibration & monitoring’. Nov. 13th , 2009 1 Nicolo Cartiglia, INFN, Turin, Italy 1 ECAL Intercalibration Problem: the same photon (or electron) gives a different answer (in ADC counts) depending upon the crystals it hits. • each crystal has a specific light yield • each photodetector has its specific gain (important in the endcaps) => poor resolution Solution: find 75848 coefficients which make every crystal answer in the same way 2100 ADC 2000 ADC Nov. 13th , 2009 Photons with CMS 2 Nicolo Cartiglia, INFN, Turin, Italy Toyoko Orimoto, 2 ECAL monitoring The calorimeter response varies due to many factors: Temperature: • Crystal light yield changes -2.1%/C • Barrel photodetectors (APD) -2.4%/C Magnetic field: • Endcaps photodetectors (VPT) Rate: • Endcaps photodetectors (VPT) Radiation: • Crystals Solution: a very powerful monitoring system which has 4 lasers, 2 sets of LED flashers and an almost crystal-by-crystal temperature monitoring system Nov. 13th , 2009 3 Nicolo Cartiglia, INFN, Turin, Italy 3 ECAL Detector Design 6.4m Barrel (EB): • 61200 crystals • 36 Supermodules (SM), each 1.7k crystals Endcap (EE): • 14648 crystals • 4 Dees • SuperCrystals of 5x5 xtals Nov. 13th , 2009 2.6m 1 Endcap Super-Crystal 1 Super-Module 1 Dee Pb-Si Pre-shower 4 Nicolo Cartiglia, INFN, Turin, Italy 4 Crystal production Crystals are grown in ingots (in Russia and China) and then cut into the right shape. Each crystal is different, with a different value of transparency and light yield Nov. 13th , 2009 Nicolo Cartiglia, INFN, Turin, Italy 5 Intercalibration & Energy resolution ‘Energy resolution’: how well do we reconstruct signals as a function of energy? Noise term: For every calorimeter we have: •Electronic (pre-amps,APD) •Pile-up s = a √E + b +cE Measured: s = 2.8% √E + 125 MeV + 0.3% E It dominates at high energy, so it should be kept small Stochastic Term: Constant term: •Photostatistics •Sampling (not for ECAL!) •Gain stage •Calibration & intercalibration •Rear leakage •Light yield non-uniformity Nov. 13th , 2009 Nicolo Cartiglia, INFN, Turin, Italy 6 From ADC to GeV Calibration aims at the best estimate of the energy of e and ’s Energy deposited over multiple crystals: Ee/ = Fe/ G i ci Ai [ +EES ] • Amplitude in ADC counts Ai • Intercalibration: uniform single channel response to a reference ci • Global scale calibration G • Particle-specific corrections (containment, clustering for e/’s) Fe/ • Preshower included in the sum in endcaps There’s inter-play across the different terms and a strategy to dis-entangle Nov. 13th , 2009 Nicolo Cartiglia, INFN, Turin, Italy 7 Present status of ci Intercalibration has been achieved in several ways, with different precision: BARREL: - Using data collected in the laboratories (all): Crystal response, APD gain, electronics constants: 4.5-6% - Cosmic ray (all): expose each SM to cosmic rays: 1-2 % - TestBeam (11 SM): electrons at a given energy in each crystal ~ 0.3 % ENDCAP: Using data collected in the laboratories (all): Crystal response, VPTgain, electronics constants. Production: 9%, Pre-production:15% - Beam splash (all): expose each Dee to muons: 15 % - TestBeam (450): electrons at a given energy in each crystal < 1 % Nov. 13th , 2009 Nicolo Cartiglia, INFN, Turin, Italy 8 What if LHC starts tomorrow Zee width EB Hγγ width EB EE • Performance acceptable for most physics in EB, nearly in EE → Target: • Target precision: 0.5% set by H benchmark channel • Approach a.s.a.p. in view of resonances Nov. 13th , 2009 Nicolo Cartiglia, INFN, Turin, Italy 9 Next step: in situ intercalibration Once we will be taking data we will exploit several channels to bring intercalibration coefficient to a much higher precisions: symmetry: based on the phi invariance, actually severely more complicated that it looked on the beginning (Stefano, Margherita). Statistically limited after a few hours of data taking. Goal: 1-2% in barrel, a few in the endcaps po mass: huge rate, 1 week at 2*1030. Goal: 0.5 % in barrel, a few in the endcap Z mass: needs good luminosity… Nov. 13th , 2009 Nicolo Cartiglia, INFN, Turin, Italy 10 In situ strategy • Derive intercalibrations ci from phi-inv. and p0/η • Fix absolute scale G and corrections (η, ET and cluster shape dependent) Fe/ with electrons from Ze+e• ES calibration (mip) and EE-ES inter-calibration • Long-term also other channels: isolated electrons Weν • There’s sufficient redundancy of calibration sources to disentangle interplay between G/Fe/ and ci : Ee/ = Fe/ G i ci Ai → Validation and combination of calibration sets • Release new sets for reconstruction as long as precision improves. Further sets for monitoring. Nov. 13th , 2009 Nicolo Cartiglia, INFN, Turin, Italy 11 Monitoring Il nostro calorimetro cambia la risposta per varie ragioni: • Temperatura: sia i cristalli che gli APD diminuiscono la risposta (luce o guadagno) se la temperatura aumenta (la combinazione dei due è -3.8%/C) • Irradiazione: i cristalli si ingialliscono a causa del danno da radiazione, tuttavia un pochino recuperano… • Fluenza: i VPT cambiano la risposta quando sono sottoposti ad un flusso continuo di particelle, quindi durante il ‘fill’ perdono brillantezza, ma poi la recuperano nell’interfill • Flusso totale: i VPT perdono brillantezza tanto più carica viene depositata sul loro catodo Soluzione: un sistema di laser/led che continuamente spara segnali ‘calibrati’ nei cristalli per monitorare la loro risposta. Nov. 13th , 2009 Nicolo Cartiglia, INFN, Turin, Italy 12 LASER Monitoring System Hardware APD PN APD Laser light sources Light distribution system (fibers, optical switches, diffusing spheres, etc.) Very stable PN-diodes used as reference system (MEM) Precision pulsing system for electronics calibration (separate hardware for MEMs) LED pulsing system for the EE, injecting into level 1 fan-out 4 Nov. 13th , 2009 VPT Nicolo Cartiglia, INFN, Turin, Italy 13 Stability of the ECAL response: Crystal transparency ECAL response will vary, depending on dose rate with a sequence of crystals transparency drops and recoveries rel. Crystal response Simulation of transparency: 2010 run: transparency change expected in innermost crystals of EE assuming ‘Classic 31 luminosity will reach L = 10 cm-2VPT s-1 effect’ induced by LHC on/off η=0.92 @ L = 2 x 1033cm-2s-1) Scenario comparable to (ECAL TDR): η=3 @ 1031cm-2s-1 changes in cathode current; mitigated by LED constant pulsing to limit current excursions: on average 1% • Transparency variation measured via response R/R0 to blue laser pulses injected in each channel in the LHC abort gap • Correction to crystal energies proportional to: (R/R0 )α • with α=1.5 BCTP crystals, α=1 SIC crystals Nov. 13th , 2009 Nicolo Cartiglia, INFN, Turin, Italy 14 Stability of the ECAL response: VPT gain Peak (VPT/PIN) 1.00 normalised Rel. VPT gain 1.01 Long term ageing: irrelevant in 2010 Rel. VPT gain ‘Classic VPT effect’ induced by LHC on/off changes in cathode current; mitigated by LED constant pulsing to limit current excursions: on average 1% 0.99 0.74 Black: load=10kHz, <IC>~0.25nA; 46 days h=2.1 and L=2.5*1033cm2s-1 Grey : load=20kHz, <IC>~1.0nA; 134 days h=2.1 and L=1034cm2s-1 0.72 0.70 0.68 0.66 0.64 0.62 ~25% 0.60 0.58 0.98 0.56 0.54 0.97 0.0 1.0 2.0 3.0 4.0 5.0 6.0 7.0 Incremental charge at Cathode (mC) 0.96 0 1 2 3 4 5 6 7 Elapsed Time (days) Response to blue laser/LED and orange LED sensitive to VPT gain changes Correction to crystal energies simply proportional to monitored change (α=1) Nov. 13th , 2009 Nicolo Cartiglia, INFN, Turin, Italy 15 8.0 Speriamo bene… • • Ci sono circa 30 persone che lavorano alla calibrazione e monitoraggio di ECAL Per ora sembra che riusciremo a farlo… Nov. 13th , 2009 Nicolo Cartiglia, INFN, Turin, Italy 16