 -bin Number Tower Calibration (ch/GeV) Desired E T matched gain s  =1.0  =2.0 from electrons slopesMIPs EEMC Towers Calibration Run 3 p+p Used 4 methods.

Slides:



Advertisements
Similar presentations
STAR Status of J/  Trigger Simulations for d+Au Running Trigger Board Meeting Dec5, 2002 MC & TU.
Advertisements

EEMC Calibration in 2004 MIP signature w/ SMD Absolute gains for SMD, pre/post-shower, towers HV setup scheme for 2005 running Jan Balewski, IUCF Joint.
Measurement of the inclusive jet cross section in p+p collisions at E CM =200 GeV Mike Miller (MIT) For the STAR collaboration.
Digital Filtering Performance in the ATLAS Level-1 Calorimeter Trigger David Hadley on behalf of the ATLAS Collaboration.
Jet probes of nuclear collisions: From RHIC to LHC Dan Magestro, The Ohio State University Midwest Critical Mass October 21-22, 2005.
INTRODUCTION TO e/ ɣ IN ATLAS In order to acquire the full physics potential of the LHC, the ATLAS electromagnetic calorimeter must be able to identify.
Direct virtual photon production in Au+Au collision at 200 GeV at STAR Bingchu Huang for the STAR collaboration Brookhaven National Laboratory Aug
1 Hadronic In-Situ Calibration of the ATLAS Detector N. Davidson The University of Melbourne.
Analysis Meeting – April 17 '07 Status and plan update for single hadron scale check with minimum bias events N. Davidson.
FMS review, Sep FPD/FMS: calibrations and offline reconstruction Measurements of inclusive  0 production Reconstruction algorithm - clustering.
Performance of the PHENIX Muon Tracking System in Run-2 Ming X. Liu Los Alamos National Lab (for the PHENIX Collaboration) –Detector Commissioning –Detector.
1 Shower maximum detector (SMD) is a wire proportional counter – strip readout detector using gas amplification. SMD is used to provide a spatial resolution.
Intercalibration of the CMS Electromagnetic Calorimeter Using Neutral Pion Decays 1 M. Gataullin (California Institute of Technology) on behalf of the.
06/03/06Calice TB preparation1 HCAL test beam monitoring - online plots & fast analysis - - what do we want to monitor - how do we want to store & communicate.
W  eν The W->eν analysis is a phi uniformity calibration, and only yields relative calibration constants. This means that all of the α’s in a given eta.
Some notes on ezTree and EMC data in MuDst Marco van Leeuwen, LBNL.
Simulation Calor 2002, March. 27, 2002M. Wielers, TRIUMF1 Performance of Jets and missing ET in ATLAS Monika Wielers TRIUMF, Vancouver on behalf.
Future  G Measurements at STAR Renee Fatemi University of Kentucky RHIC Spin Meeting, LBNL, November 21st 2009.
STAR Analysis Meeting, BNL, Dec 2004 Alexandre A. P. Suaide University of Sao Paulo Slide 1 BEMC software and calibration L3 display 200 GeV February.
Real data reconstruction A. De Caro (University and INFN of Salerno) CERN Building 29, December 9th, 2009ALICE TOF General meeting.
Thomas Jefferson National Accelerator Facility Page 1 EC / PCAL ENERGY CALIBRATION Cole Smith UVA PCAL EC Outline Why 2 calorimeters? Requirements Using.
 production in p+p and Au+Au collisions in STAR Debasish Das UC Davis (For the STAR Collaboration)‏
Preliminary analysis of p-Pb data update n. 6 Lorenzo Bonechi LHCf Catania meeting – 19 December 2013.
STAR Collaboration Meeting, Nantes Alexandre A. P. Suaide Wayne State University Slide 1 EMC Commissioning for the run Review of last.
Jet Calibration Experience in CDF Beate Heinemann University of Liverpool -CDF calorimeter -Relative Calibrations -Absolute Calibration -Multiple Interactions.
STAR Collaboration Meeting, BNL, Feb 2005 Alexandre A. P. Suaide University of Sao Paulo Slide 1 BEMC software update L3 display 200 GeV February.
1 Lead glass simulations Eliane Epple, TU Munich Kirill Lapidus, INR Moscow Collaboration Meeting XXI March 2010 GSI.
Dec.11, 2008 ECL parallel session, Super B1 Results of the run with the new electronics A.Kuzmin, Yu.Usov, V.Shebalin, B.Shwartz 1.New electronics configuration.
08-June-2006 / Mayda M. VelascoCALOR Chicago1 Initial Calibration for the CMS Hadronic Calorimeter Barrel Mayda M. Velasco Northwestern University.
PHOS offline status report Dmitri Peressounko ALICE offline week,
The Electromagnetic Calorimeter – 2005 Operation J. Sowinski for the Collaboration and the Builders Indiana Univ. Michigan State Univ. ANL MIT BNL Penn.
LM Feb SSD status and Plans for Year 5 Lilian Martin - SUBATECH STAR Collaboration Meeting BNL - February 2005.
FTPC status and results Summary of last data taken AuAu and dAu calibration : Data Quality Physic results with AuAu data –Spectra –Flow Physic results.
STAR J/  Trigger in dA Manuel Calderon for the Heavy-Flavor Group Trigger Workshop at BNL October 21, 2002.
Forward Carriage Commissioning CLAS Collaboration Meeting 6/19/2015CLAS12 CalCom Status Update1 ECAL PCAL FTOF Panel 1A FTOF Panel 1B Detector Status PMT.
Mike Miller First measurement of the inclusive jet cross section in p+p collisions at E CM =200 GeV M.L. Miller (MIT) Motivations: 1.Baseline for inclusive.
STAR Collaboration Meeting, BNL – march 2003 Alexandre A. P. Suaide Wayne State University Slide 1 EMC Update Update on EMC –Hardware installed and current.
STAR Analysis Meeting, BNL – oct 2002 Alexandre A. P. Suaide Wayne State University Slide 1 EMC update Status of EMC analysis –Calibration –Transverse.
STAR Collaboration meeting, Nantes Alexandre A. P. Suaide Wayne State University Slide 1 EMC analysis update Just to remember … What we have done.
E-EMC developments and plan Jan Balewski IUCF, Indiana Detector status Run 3 goals Calibration Software status STAR Analysis Meeting BNL, October
Longitudinal Spin Asymmetry and Cross Section of Inclusive  0 Production in Polarized p+p Collisions at 200 GeV Outline  Introduction  Experimental.
ScECAL Beam FNAL Short summary & Introduction to analysis S. Uozumi Nov ScECAL meeting.
Search for High-Mass Resonances in e + e - Jia Liu Madelyne Greene, Lana Muniz, Jane Nachtman Goal for the summer Searching for new particle Z’ --- a massive.
Some feedbacks from DRS data analysis (very preliminary) F. Scuri - I.N.F.N Sezione di Pisa RD52 – Collaboration Meeting – Pavia, March 12, 2013 F. Scuri.
Quality assurance for TPC. Quality assurance ● Process: ● Detect the problems ● Define, what is the problem ● What do we expect? ● Defined in the TDR.
 0 life time analysis updates, preliminary results from Primex experiment 08/13/2007 I.Larin, Hall-B meeting.
Outline Motivation The STAR/EMC detector Analysis procedure Results Final remarks.
Hadronic resonance production in Pb+Pb collisions from the ALICE experiment Anders Knospe on behalf of the ALICE Collaboration The University of Texas.
Online Consumers produce histograms (from a limited sample of events) which provide information about the status of the different sub-detectors. The DQM.
1 EMCAL Reconstruction in Pass pp 900 GeV 29/03/2010 Gustavo Conesa Balbastre.
Elliptic flow of D mesons Francesco Prino for the D2H physics analysis group PWG3, April 12 th 2010.
EEMC Photons Pibero Djawotho (IUCF) Wednesday, October 17, 2007 STAR Analysis Meeting (BNL)
Vertex Reconstruction for High Luminosity pp Running at STAR STAR-Spin luminosity requirements Method of the vertex reconstruction Application to the pileup.
Toward a  +Jet Measurement in STAR Saskia Mioduszewski, for the STAR Collaboration Texas A&M University 1.
Inclusive  0 Production in Polarized pp Collisions Using the STAR Endcap and Barrel Electromagnetic Calorimeters Jason C. Webb for the STAR Collaboration.
R. Croft, Exclusive Diffractive Higgs Signal at L1, Jan 2005 Diffractive Higgs Events in the L1 Trigger ( Work in progress ) Richard Croft, University.
EEMC STAR Jan Balewski, IUCF, Indiana STAR Collaboration Meeting MSU, August 2003 Upper Structure Mounted 8/1/2003 Run 3 hardware calibration.
Analysis Meeting, November 9-11, 2003 Manuel Calderón de la Barca Sánchez Heavy Flavor Working Group Heavy Flavor in ‘04: Prospects for J/ . Heavy.
1 Methods of PSD energy calibration. 2 Dependence of energy resolution on many factors Constant term is essential only for energy measurement of single.
Direct Photon v 2 Study in 200 GeV AuAu Collisions at RHIC Guoji Lin (Yale) For STAR Collaboration RHIC & AGS Users’ Meeting, BNL, June 5-9.
Custom Classes DetectorShapeView2D: Detector mouseover callbacks (default is mouse click). EventControl:
June 4, 2009 STAR TPC review Estimation of TPC Aging Based on dE/dx Measurements Yuri Fisyak.
Feb C.Smith UVA EC energy calibration – g13 pass0 For pass0 data were cooked with CALDB calibration constants reset to nominal 10 channels / MeV.
Elena Bruna Yale University
CLAS12 software workshop
Yuxi Pan University of California, Los Angeles
Commissioning of the ALICE-PHOS trigger
J/Y Simulations for Trigger
Inclusive p0 Production in Polarized pp Collisions using the STAR Endcap Calorimeter Jason C. Webb, Valparaiso University, for the STAR Collaboration Outline.
Presentation transcript:

 -bin Number Tower Calibration (ch/GeV) Desired E T matched gain s  =1.0  =2.0 from electrons slopesMIPs EEMC Towers Calibration Run 3 p+p Used 4 methods isolated slopes - relative Tracked MIPs 2-Tower  0 ’s Electrons Methods agree but hardware calibrated to ~constant E not E t J. Balewski, P. Zolnierczuk, J. Webb

Relative Gains from MIP’s – ‘03 Set HV by matching slopes Require no signal in adjacent towers Requires 200 kevts Furnishes relative gain of each tower Have performed 4 iterations this year HVs should not change in Au-Au Used L3 tracks – ’04? Require track to stay in tower Full ’03 p-p data set gives gain for individual towers (14 Mevt) Sampling fraction of 5.0% agrees with electron and  0 abs. gain. Slopes Use tracked MIPs for 1.1  1.4 

EEMC Response to Tracked Electrons – ‘03 Use window on pions over same p range to estimate background EEMC response Use TPC dE/dx vs. p to select track region where electrons are (slightly) dominant. Requires full p-p data set to get  averaged absolute gains for each  Does not work at large  With presently available statistics, this gives (55 ± 5) channels/ GeV on ‘calibration’ tower 5TB09. This compares well with 52 channels/GeV determined from MIP peak location for 5TB09, and with (58 ± 2) channels/GeV determined from reconstructed  0 invariant mass.

EEMC (Tower Only)  0 Reconstruction – ’03 Two-cluster invariant mass spectra show clear  0 peak after subtraction of mixed-event background. Events sorted according to  bin of the higher-energy cluster. Data here triggered by EEMC high-tower in p+p. Relative gains within each  bin taken from MIP response. Absolute gains adjusted to place reconstructed  0 peak at “correct” mass. “Correct” mass determined from simulations. Requires full p-p data set to get  averaged gains Occupancy in Au-Au may give lower fraction of useful events than p-p Underway for ’04 data simulated measured }( ) 2 mm m  =2  =1

1 st  0 s in EEMC from ’04 Data!

Cluster Finder under Development Enhanced  0 reconst. in 4 sectors with SMD –Better position resolution –Better understood energy sharing –Extends range in p t of useful  0 s 4.5 GeV  f     SMD Strip # - within tower ADC Au-Au event from ’04 – HT triggered

Tower Cluster Finder on a recent Au-Au event EEMC in database Mapping from channel and crate to detector element name Geometry hard coded since unlikely to change Pedestals loaded and in use Gains – structure exists 32 bit status word Sector based Flavors implemented GUI or program to edit or load

Significant effort into online QA plots for EEMC has proven essential to bringing detector online and debugging problems ADC spectra for 2 crates ADC spectra for 2 MAPMT boxes DSM input vs. output H. Spinka

EEMC Software Jobs and Workers* *I am bound to leave someone out: My apologies IUCF Jan Balewski a (Coordinator) Renee Fatemi b Jason Webb c 1 more post-doc? 2-3 students by summer d Note: -Piotr Zolnierczuk e ANL Bob Cadman f MIT g Post-doc Students Valparaiso U Gopika Sood j Paul Nord k CalTech Dave Relyea h Kent State Wei-Ming Zhang m EEMC Infrastucture Clustering for towers and SMD c Correlation of TOW, SMD, PPS & tracking ckm Extend tracking to  > 1.4 g e/h discrimination for sectors w/ SMD Noise rejection in clustering  0 reconstruction & inv. mass ac L3 Display k Adapt recent software to Root4Star ac Fill database abc Determine neutral energy in EEMC Commiss./Calibration Online QA a,Spinka Status of towers and strips Tower gains: MIPS, e,  0ace SMD strip gains fm PPS gains Jet trigger during p-p b Phys. Analysis & Simul. High-p t  0,  spectra in EEMC High-p t e spectra in EEMC Inclusive High-p t  ’s Jet trigger bias in p-p b Forward tracking upgr. sims. g ’04 p-p analysis Slow simulator Simple EEMC response for sims. bg Pileup in p-p