eemc perspectives @ star

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EEMC perspectives @ STAR Jan Balewski, IUCF, Indiana STAR Collaboration Meeti MSU, August 2003 per Structure Mounted 8/1/2003 • Run 3 • hardware • calibration • trigger • software • Run 4 • expectations • goals

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EEMC perspectives @ STAR. Run 3 hardware calibration trigger software Run 4 expectations goals. Jan Balewski, IUCF, Indiana. STAR Collaboration Meeting MSU, August 2003. Upper Structure Mounted 8/1/2003. Instrumentation for pp Run 3. Pb Scint sampling calorimeter - PowerPoint PPT Presentation

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Page 1: EEMC perspectives @ STAR

EEMC perspectives @ STAR

Jan Balewski, IUCF, Indiana

STAR Collaboration MeetingMSU, August 2003Upper Structure Mounted 8/1/2003

• Run 3 • hardware• calibration• trigger• software

• Run 4• expectations• goals

Page 2: EEMC perspectives @ STAR

Instrumentation for pp Run 3• Pb Scint sampling calorimeter• 21 radiation lengths• 240 of 720 projective towers• Depth Segmentation

– 2 preshower layers– High position resol. SMD– Postshower layer (no readout)

• L0 trigger:– high tower (working)– jet patches (problems)

8

765

preshower

SMDU,V

post

6 GeVelectron

Page 3: EEMC perspectives @ STAR

EEMC Calibration Summary from EEMC Calibration Summary from 2003 STAR p+p Data2003 STAR p+p Data

Three completely independent absolute calibration approaches agree at the 10-20% level:

1) MIP peak location, assuming 5.0% sampling fraction (as per simulations);

2) reconstructed 0 invariant mass from EEMC towers alone;

3) p/E from TPC-tracked electrons to EEMC.

4) “Isolated MIP slopes” used online gave reasonable gain matching for different bins at given .

Note:

0 reconstruction (after correction for simulated systematic shift for very asymmetric decays) and MIP peaks give consistent relative gains vs. .

“Bootstrapping” approach, based on cosmic rays, 60Co source, and isolated MIP’s did not achieve desired ET matching or absolute gains!

Following data from: R. Fatemi, J.Webb, P.Zolnierczuk, and J.B. THANKS !

Page 4: EEMC perspectives @ STAR

Relative Gains from MIP’sRelative Gains from MIP’s

For 1.0 1.5 , use MIP’s tracked from TPC to EEMC, where track predicted to enter and exit same tower. Landau fit to observed peak shape determines absolute gain of each tower illuminated, using 5.0% sampling fraction to convert to equivalent shower energy.

=1.5

=1.0• L3 tracks & vertex used off-line

For towers where clear MIP peak not visible, or tracking not available, use slope of tower ADC spectrum in anti-coincidence with neighboring towers as measure of relative gain. This is correlated very well with MIP peak location where both available.

Pre calibrationused in pp Run 3

Page 5: EEMC perspectives @ STAR

EEMC Response to Tracked EEMC Response to Tracked ElectronsElectrons

Take relative tower gains from MIP’s, and adjust overall absolute calibration constant to match EEMC E to TPC p.

With presently available statistics, this gives (55 ± 5) channels/ GeV on ‘calibration’ tower 5TB09.

Use TPC dE/dx vs. p to select track region where electrons are (slightly) dominant.

Use window on pions over same p range to estimate background EEMC response

L3 tracks, vertex, dE/dx used off-line

Page 6: EEMC perspectives @ STAR

Electrons Trigger EHT-1,2

p/E1

elec

tron

s

Electron Energy reco in EEMC (GeV)

2

MinB trigger(2 M eve)

EHT1 trigger(540 K eve)

EHT2 trigger(140 K eve)

E=3.3 GeV

E=5.5 GeV

L2 Enrichment (potential)• select trig tower and

• require pre1 ~pre2 MIP• veto postshower

• not tested with M-C• no data to play with• factor 10 would do

Identified electrons w/ bckg

used K=50 ch/GeV

0 10

0 10

Page 7: EEMC perspectives @ STAR

MinBTriggerdata

00 Total Energy Total Energy 00 Energy Sharing Energy Sharing-- Invariant MassInvariant Mass

raw

mix

diff

data ‘diff ’

M-C pi0E=2 GeV

<M>=149 MeV =69 MeV

001

2

12 E1- E2

Z00= —––– E1+ E2

invM12* (E1* E2)

EEMC (Tower Only) EEMC (Tower Only) 00 ReconstructionReconstruction

Cuts:• seed >0.7 GeV• seed/cluster >0.7

EHT-1&2Triggerdata

data ‘diff ‘

M-C pi0E=8 GeV

M-C pi0E=6GeV

invM (GeV) Reco ener (GeV) Z

<M>=192 MeV =45 MeV

Page 8: EEMC perspectives @ STAR

00 1

2

MinB trigger yields symmetric decayed 0

12

E1- E2

Z00= —––– E1+ E2

invM12* (E1* E2)

Reconstruction of Reconstruction of 00 with Limited Angular with Limited Angular ResolutionResolution

Seed-1

Seed-2

0 0.7 GeV Tower energy

E’1= E1

E’2= E1 – +

12*{ E1* E2 (E1- E2)} m00

Z0 0 0

Seed-1

Seed-2

0 0.7 Tower energy

E’1= E1 – E1

3.5 GeV

E’2= E2 + E1

Seed thr

trigger thr

12*{ E1* E2 + E12} m00 *(1+ E1/ E2)

Z0 0 0.8

2 GeV2 GeV

00

E1=7

E2=1

8 GeV8 GeV

00

High Tower trigger yields asymmetric decayed 0

Mostly overestimated

Overlaperror

E1= E2= 1

=7

0

Cuts:• seed >0.7 GeV• seed/cluster >0.7

Page 9: EEMC perspectives @ STAR

-dependent Gains from Reconstructed -dependent Gains from Reconstructed 00 Events sorted according to bin of the higher-energy cluster.

Data here triggered by EEMC high-tower in p+p.

“Correct” mass determined from simulations, which take account of geometric effects and imperfect E sharing between clusters for the very asymmetric (E1 / E2 7:1) decays that satisfy high tower trigger + tower min. open.

Relative gains within each bin taken from MIP response. Absolute gains will be adjusted to place reconstructed 0 peak at “correct” mass.

Simulated pi0 E=8 GeVMeasured w/ SF=50 ch/GeV

( ) 2invMM pi0

=2.0

=1.0

Page 10: EEMC perspectives @ STAR

-bin Number

Tow

er C

alib

rati

on (

ch/G

eV)

Desired ET matched gains

=1.0

=1.0

=2.0

=2.0

fromelectrons

slopes MIPs

EEMC Towers Calibration Run 3 p+pTower Gains in Run 3• flat in energy ~50-60 ADC ch/GeV• known from MIP or slope 10% (stdev) • HV matched 20% (stdev)

Goal ‘slopes‘from thesource scan

Slopes ~ -1/gain

=1.0=2.0

Page 11: EEMC perspectives @ STAR

EEMC Trigger in Run 3

ADC value

tow

er I

D

EHT-13.3 GeV

EHT-25.5 GeV

High Tower Trigger OK• EHT1 @ E=3.3 GeV

• slow 600 K events• fast 300 K events

• EHT2 @ E=5.5 GeV • slow 140 K events

Jet Trigger problems• ped close to N*16 – fixed in FEE• correlated noise N*256 – veto Ejet>200 GeV• correlated ghost ped - ?• 1% data corruption - ?

ADC value

CRATE 3, FEE CH 42 no detector !

GhostPed

TP input to DSM

TP

ID

No hotchannels

Page 12: EEMC perspectives @ STAR

EEMC (Tower) Database for Run 3

On-line• monitor HV every 5 minutes• record any change for any tube

Days in 2003

No change May 1-June 15

Plot for 20 tubes

HV

(V

)

Off-line• map of FEE channel vs. tower• gains, one set from day 120+• ped, new set each RHIC fill,

(changes below 1 ADC ch)

• available in root4star

Page 13: EEMC perspectives @ STAR

Software & Simulations (done)Software • EEMC geometry in GSTAR (Oleg Rogachevski)• fast simulator for towers/ pre/ post/ SMD• DAQ reader (tower energy, Herb)• DAQ ezTree ( Piotr)• StEvent (Akio)• StEvent muDst (Alex)

Data sets• DAQ pp200 (towers):

• 2 M minB events• 1 M EHT-1/2(available in ezTree format)

• M-C PYTHIA, geom2003:• 1.3 M minB• 0.5 M partonic pT>5 GeV• 0.5 M partonic pT>15 GeV

Page 14: EEMC perspectives @ STAR

2

3

4

5

6

1

1ch

16ch

1 2 3 4 5 6 SMD 7 8 9 10 … 24

Incident particles

MAPMTPre1,2,Post

PMTtower

16 ch

MAPMT SMD strips

Layer:

• L0 trigger:– high tower– jet patches

• readout– 720 towers– 5/12 pre/post– 5/12 SMD

Run 4 InstrumentationView from IRtowards West(along Z-axis)

South North

West

Page 15: EEMC perspectives @ STAR

Run 4 Calibration Plan

Commissioned 240 towers• fix ~10 dead ch

• change gain to ET-match with LED

• check gains with MIP and pi0

New 480 towers• before beam

• set initial HV based on known gains• verify all channels with LED/laser

• in beam (early)• use ‘slopes’ , gain match 50%

(ET-match to calibrated towers )

• use pi0 in dedicated run to gain match 10%• off-line

• MIP, pi0, electrons

New pre- post- shower, SMD• verify mapping: LED (or sourse) • set initial HV based on known gains • in beam set gains with MIP • for SMD try pi0• pre/post: gains set high to see 1.e.e. ?

Goals:• towers 10% (used in trigger)• Pre/post/SMD 50% (in the range of ADC)

Page 16: EEMC perspectives @ STAR

Physics Goals of Run 4• contribute to jet trigger @ eta>1• contribute to J/Psi and/or Upsilon in AuAu• trigger on high energy gamma• reco pi0 up to ~20 GeV• deal with pileup

Page 17: EEMC perspectives @ STAR
Page 18: EEMC perspectives @ STAR

Detailed Software Tasks• Slow control: (Wei Ming/Valpo) - gui+VME HV sys - STAR alarm: HV & FEE ped - laser control - main EEMC gui – DSM, Tower, SMD - documentation for shifts - ped loaded to trigger FEEonline DB - MAPMT box temperature• SMD/Pre/Post Commissioning: (Scott/Steve )• online histos : (Dave and Hal) - define & implement (Paniatkin plots)• display : (Paul Nord?/Valpo) - EEMC on L3 screen or- automate tower+SMD+pre/post+track (online)- (predict) fired SMD strips with LED pulser

• calibration : (Piotr/Jan/Wei Ming) - Pedestals: smd/pre/post - duplicate tower code - Gains: pre/post - duplicate tower code for MIP SMD – MIP finder code exist

write to DB, test

• off-line database (Jan/Piotr) - pre/post : duplicate tower info - SMD : as tower + box mapping

-calibration code (SMD) (Wei Ming) - access in root4star ?• L2 programming : (Renee/Steve/Jason) - enriched calibration trigger (pi0/e/MIP)• tracking at eta>1.5 : (MIT/Jason) - not existing, use ITTF • merge hits: (ANL/Valpo/Piotr)

- pi0 reco at ~20 GeV - pi0/gamma/hadrons ID

• EEMC contribution to jet energy (Renee)• trigger simulator (Renee)

STAR tasks list:www.star.bnl.gov/STAR/Comp/general/task.html

Page 19: EEMC perspectives @ STAR

Unsupported Software Tasks

• pre/post/SMD data StEvent• pi0 reco : port FPD algo (tw+smd)• EEMC slow simulator• EEMC embedding • vertex reco :

- integration with ITTF- pileup : B+E-EMC, SVT

• display : EEMC on L3 plasma-screen