DHCAL - Resolution (S)DHCAL Meeting January 15, 2014 Lyon, France Burak Bilki, José Repond and Lei Xia Argonne National Laboratory.

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Presentation transcript:

DHCAL - Resolution (S)DHCAL Meeting January 15, 2014 Lyon, France Burak Bilki, José Repond and Lei Xia Argonne National Laboratory

2 Resolution for Pions Calibration Improves result somewhat (no dramatic effect) Monte Carlo prediction Around 58%/ √ E with negligible constant term Saturation at higher energies → Leveling off of resolution → Can be mitigated with software compensation

Introduction to SW Compensation Single particle energy resolution of a traditional calorimeter can be optimized by hardware/software compensation – Equalize EM and Hadronic responses -> e/h ~ 1 The DHCAL is quite a unique/different device – Non-linear response for EM shower Measured energy of a 10 GeV photon E(10) E(10) ≠ E(5) + E(5) ≠ E(2) + E(2) + E(2) + E(2) + E(2) Correction can be applied for single EM showers No obvious way to correct for pi0’s generated in hadronic showers – Hadronic response close to linear -> Ratio of EM to hadronic response changes with energy – Software compensation not likely to be very successful without first taking care of the non-linearity of the EM response 3

Linearizing the EM response I The non-linear response of EM showers is due to finite readout pad size  multiple particles hitting same pad  saturation Need ways to account for multiple particles on the same pad – Assumption: Hit density (hit fraction in a given local space) is related to the local particle density (Density weighted calibration proved good correlation between hit density and local particle density) – Start with simple hit density definition d9: number of hits in the surrounding 3pad x 3pad area, centered on the hit being studied (d9 = 0 – 8) – Start with MC simulation for Fe absorber setup RPC response: RPC_sim_4 (single exponential) – not the best… Positron sample: 2, 4, 6, 8, 10, 12, 16, 20, 25, 32, 40, 60 (GeV) Pion sample: 2, 4, 6, 8, 10, 12, 16, 20, 25, 32, 40, 60, 80, 100 (GeV) 4

Linearizing the EM response II Chose two sets of positron energy points, adjust weights for each D9 bin to achieve linear response – Set I (wt1): 2, 6, 10, 16, 25 (GeV) – Set II (wt2): 2, 6, 16, 32, 60 (GeV) – Target response: hits/GeV (arbitrary) High weights for isolated hits Low weights for medium density: mostly due to hit multiplicity ~ 1.6 Very high weight for high density bins: correction for saturation Everything as expected 5

Positron response after weighting Things are exactly as expected: Linearity significantly improved wt2 gives better linearity in larger energy range than wt1 6 Fits to power law (β =1 means linear)

Positron resolution after weighting Non-linearity correction is included (this is very important!) Positron energy resolution modestly improved (2 – 11%) Not much difference between wt1 and wt2 All energy resolutions were calculated from full-range Gaussian fit Fit at low energies are not very reliable 7

Pion response Pion linearity (no weighting) is much worse than in data (most likely due to inaccurate positron simulation) Linearity fits are not as good as the positrons * Applied leakage cut: no more than 10 hits in tail catcher 8

Pion resolution Pion resolution and linearity are both greatly improved in (not very good) simulation: 10 – 50% At higher energies, distributions become much more symmetric after weighting Example: 60 GeV response 9

Pion vs. Positron response Before weightingAfter weighting Pion and Positron responses are brought closer by weighting, but not equal yet (weighting changes both pion and positron responses) Room for software compensation: work in progress (pretty optimistic on further improvement) 10

Next step: data Burak kindly provided Fe data sample – Particle identification and quality checks were all done – Hit density, calibration constants were pre-calculated – Positron energy: 2, 4, 6, 8, 10, 12, 16, 20, 25, 32, 40 (GeV) – Pion energy: 2, 4, 6, 8, 10, 12, 16, 20, 25, 32, 40, 50, 60, 120 (GeV) – Only used first 10K events (if there are that many) of each energy point Weights were optimized with 2 sets of positron data (calibrated) – Set I (wt1): 2, 4, 6, 8, 10, 12 (GeV) – Set II (wt2): 2, 4, 6, 10, 16, 25 (GeV) – Weighting is based on calibrated data (density calibration) Set I energies are probably all too low 11

Positron response It would probably be better if we had higher energy positron data 12

Positron resolution Similar to simulation: no big gain for positrons 13

Pion response As usual, pion fits are not very good compare to positron fits 120 GeV points are systematically low  Excluded from fits Data points before calibration are quite scattered, fit value pulled up by 60 GeV point Calibrated points (including the weighed points) are much smoother Fit to entire distribution including tails (leading to higher apparent saturation in calibrated data) 14

Pion resolution Don’t see nearly as much improvement, but still systematically improved Nhits distribution much more symmetric to start with Weighting makes distribution more symmetric, but a long tail remains Example: 60 GeV 15

Possible reason I: data quality issue? See long high-end tail in positron sample Long low-end tail in pion sample Both are absent in simulation Could it be contamination? The long tails seem to be a limiting factor for further resolution improvement 16

Possible reason II: EM response Pion simulation agrees with data below 32 GeV Positron simulation systematically lower than data and has worse linearity e/p difference larger in simulation  worse pion linearity e/p improved by weighting, in both data and simulation Software compensation should further improve data resolution 17

More density weighting It seems that things work best with very different e/p responses and very non-linear EM response One obvious place is W-DHCAL data: studies using simulated events – Electron sample: 2, 4, 6, 8, 10, 20, 30, 40, 50, 60, 80, 100 (GeV) – Pion sample: 8, 10, 20, 30, 40, 50, 80, 100, 120, 150, 180, 300 (GeV) – Weights tuned with electron energy points: 4, 10, 30, 50, 80 (GeV) 18 weights Density bin d9

Electron response Response is highly non-linear without weighting Weighting does a good job, as with the Fe-DHCAL (tuning target was 10 Hits/GeV, again, arbitrary) 19

Electron resolution As with the Fe-DHCAL, no significant improvement Fits at low energy points are not reliable 20

Pion response As usual, fits are not great as compare to electron fits 300 GeV point systematically low  Excluded from fits All high energy points are low probably due to bias from leakage cut Fit parameters are also systematically low, probably due to the above reason Nevertheless, linearity did improve significantly 21

Pion resolution Energy resolution greatly improved over large energy range: 24 – 54% Weighing improved distribution, but didn’t totally remove low end tail 22 Example: 50 GeV response

Pion vs. electron responses Before weightingAfter weighting e/h improved with density weighting Difference is still very large  ideal test bed for software compensation 23

Summary Density weighting is able to achieve close to linear EM shower response for DHCAL Using the same weights can improve linearity and energy resolution of pion showers – Significant (~ %) improvement observed with Fe-DHCAL and W- DHCAL simulation – Applying the same technique for test beam data results in somewhat more modest improvements (contamination of samples? MC simulation of em showers off?) Pion and EM shower response are still quite different after weighting – Chance for software compensation: work started Once we have the method to get optimized energy resolution for DHCAL, we should think of optimizing the DHCAL design itself… 24

25 Comparison of Resolutions Results with software compensation still has tails. Fit to 90% of entries will result in significant improvements. Results with software compensation not yet preliminary. Additional improvements very likely.