1 mtd calibration for cosmic ray triggered data in run 10 at star lijuan ruan (bnl), liang li (ut...

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1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production and Related Physics, Hefei, Anhui, China, March 30th - April 1st, 2011

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Page 1: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR

Lijuan Ruan (BNL), Liang Li (UT Austin)

04/01/2011

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Workshop on STAR MTD Production and Related Physics, Hefei, Anhui, China, March 30th - April 1st, 2011

Page 2: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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Motivation• In run year 10 STAR implemented a cosmic ray trigger to study

the performance of its several subsystems, including TPC, MTD, TOF etc.

• Because the cosmic rays are primarily muons, we were able to get rid of the hadron background from material interactions in the MTD analysis, as seen in previous studies with data from physical collisions.

• Also the cosmic ray data offers us significant amount of muon tracks with pt > 2 GeV/c, and these high momentum particles have less interaction with the material than the lower momentum particles therefore we can calculate the tracking information more precisely.

Page 3: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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The STAR Detector

Page 4: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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Muon Telescope Detector

• Since RUN 9 p+p 200 GeV period a new prototype of MTD has been installed outside the STAR magnet steels at a radius ~ 400 cm from the STAR detector center and used to take data at STAR. It is one tray with 3 long MRPC modules and each module has 6 strips.

• There are two read-outs for each strip, from the east side and west side respectively.

• This prototype utilized the same electronics as that for TOF in order to achieve a better timing resolution than that from trigger electronics.

Page 5: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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Data Set

• RUN 10 Au+Au 11 GeV fastoffline production of st_mtd data stream for Reversed Full Field

• Selected cosmic ray tiggered events with “cosmic” offline Tigger ID 310803

• Global tracks were used

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Page 6: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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QA Plots

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Pt (GeV/c) TOT (ns)

(P1-P2)/P1 Energy Loss

Page 7: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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Method

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The time difference between TOF+MTD measured time and TPC measured time is deltaT = (tTOF2 – tTPC + tTOF1)/2 – tMTD - tSteel

Zhangbu XutMTD is calculated by averaging the times from two ends of an MTD strip so that it does not depend on the hit position on the strip.

tTOF1 and tTOF2 are calibrated times associated with TOF hits due to the cosmic ray muons.

tTPC is the calculated time of flight between two TOF trays 1 and 2 with the pathlength and momentum information from TPC.

tSteel is the time of flight from MTD to TOF, also calculated with TPC information

Page 8: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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Matching• The matching between 2 halves of a muon track in TPC

requires nHitsFit>14, |eta|<1.5 and p>1 GeV/c for each half and |p1-p2|/p1<0.27, where p1 and p2 are the momenta for the two halves.

• The next step is raw matching for the TPC tracks. The requirements are nFitPoints >= 25, Pt >= 2.0 GeV/c, TpcZ < 100 cm && TpcZ > (- mrpcLength - 100 cm), TpcPhi > 0.419 && TpcPhi < 0.628, where Z is the position along the beam pipe and an MTD strip, TpcZ and TpcPhi are extroplated Z and Phi values for a track from TPC.

• Finally we do the matching between the TPC tracks and the MTD hits, requiring |TpcZ-MtdZ| < 6 cm and |TpcPhi-MtdPhi| < 0.2. MtdZ is from the timing difference between 2 ends of a strip and MtdPhi is from the center of the fired MTD strip.

Page 9: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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Position Resolutions

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deltaZ (cm)Sigma = 2.5 cm

deltaPhiSigma = 0.006 rad

Page 10: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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TOF Timing Resolution

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deltaT0 = tTOF2- tTOF1 – tTPCTOF timing resolution ~92.9 ps/sqrt(2) ~ 66 ps, close to the result in our intrinsic timing resolution study (M Shao and L Li, International Journal of Modern Physics E, Volume 16, Issue 07-08, pp. 2476-2483 (2007))The mean value is close to 0

Delta T(ns)

Page 11: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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The First T0 Offset Correction

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Delta T(ns) Delta T(ns)

First, we did a T0 offset correction for each strip. Basically we fitted the deltaT histograms with a Gaussian function and subtracted the obtained mean value from tMtd.

Page 12: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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MTD Timing Resolutions By Strip Before Calibration

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~196 ps

Page 13: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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The Slewing Correction

Secondly, we combined all channels and plotted deltaT versus averageTOT=sqrt(totMtdEast*totMtdWest). The slewing correction curve is obtained by a 4th order polynomial function fitting the Gaussian mean deltaTs for all averageTOT bins. Then the slewing correction is done by subracting the function value from tMtd according to its averageTOT value. The slewing correction is done for only TOT<22 ns because above that the statistics is poor.

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TOT (ns)

Del

ta T

(ns)

Page 14: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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The Second T0 Offset Correction

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Delta T(ns) Delta T(ns)

Delta T(ns) Delta T(ns)

A second T0 correction is done thereafter due to the observed T0 shift after the slewing correction

Page 15: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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Final MTD Timing Resolutions By Strip

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~106 ps

Page 16: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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The Final MTD Timing Resolution

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MTD+TOF timing resolution: ~109psTiming resolution from TOF: ~46ps MTD timing resolution: ~99ps

Page 17: 1 MTD Calibration for Cosmic Ray Triggered Data in RUN 10 at STAR Lijuan Ruan (BNL), Liang Li (UT Austin) 04/01/2011 1 Workshop on STAR MTD Production

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Summary

• MTD calibration for Au+Au 11 GeV fastoffline production in RUN 10 (RFF) with cosmic ray triggered events is done.

• ~109 ps timing resolution for MTD+TOF is achieved, giving ~99 ps for MTD alone.

• From this analysis, ~66 ps TOF timing resolution is demonstrated.

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Thanks!