2007 run update for star

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2007 Run Update 2007 Run Update for STAR for STAR Jeff Landgraf Jeff Landgraf For the STAR For the STAR collaboration collaboration

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2007 Run Update for STAR. Jeff Landgraf For the STAR collaboration. STAR’s BUR Goals. Expected RHIC performance From W. Fischer Doc. Ver. 6/1/06. To meet our AuAu goals we anticipate needing ~1.8 nb -1 of Delivered luminosity. STAR’s BUR Goals. - PowerPoint PPT Presentation

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Page 1: 2007 Run Update for STAR

2007 Run Update 2007 Run Update for STARfor STAR

Jeff LandgrafJeff Landgraf

For the STAR collaborationFor the STAR collaboration

Page 2: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

Expected RHIC performance

From W. Fischer Doc. Ver. 6/1/06

To meet our AuAu goals we anticipate needing ~1.8 nb-1 of Delivered luminosity

STAR’s BUR GoalsSTAR’s BUR Goals

Page 3: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

Expected RHIC performance

From W. Fischer Doc. Ver. 6/1/06

To meet our AuAu goals we anticipate needing ~1.8 nb-1 of Delivered luminosity

STAR’s BUR GoalsSTAR’s BUR Goals300ub-1 300ub-1 600ub-1 because 600ub-1 because our measurement of sampled our measurement of sampled luminosity this year doesn’t luminosity this year doesn’t include a vertexinclude a vertex

Page 4: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

Additional GoalsAdditional Goals Progress on Detector Upgrade PrototypesProgress on Detector Upgrade Prototypes

Improved Vertex Detector (VPD)Improved Vertex Detector (VPD) TPC DAQ upgrade (DAQ1000)TPC DAQ upgrade (DAQ1000) Forward Meson Spectrometer (FMS)Forward Meson Spectrometer (FMS) Muon Tracking Detector (MTD)Muon Tracking Detector (MTD) Heavy Flavor Tracker (HFT) Heavy Flavor Tracker (HFT) (PIXEL) (PIXEL)

Prepare for an eventual Low Energy Au-Prepare for an eventual Low Energy Au-Au RunAu Run Collider CommissioningCollider Commissioning Explore STAR’s Triggering CapabilitiesExplore STAR’s Triggering Capabilities

Page 5: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

Advances in STAR since the 2004 AuAu Run:Advances in STAR since the 2004 AuAu Run:

The Full Barrel The Full Barrel EMC is now EMC is now installedinstalled

The full SSD is The full SSD is now installed now installed which enhances which enhances the capabilities the capabilities of the SVTof the SVT

Improved Improved capability to capability to trigger on a trigger on a narrow vertex narrow vertex using the new using the new vertex position vertex position detector (VPD)detector (VPD)

Shielding was Shielding was added to remove added to remove backgrounds backgrounds from the Barrel from the Barrel EMCEMC

L2 Trigger L2 Trigger SystemSystem

Page 6: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

A Minimum Bias program to Measure D’s using the SSD / SVT A Minimum Bias program to Measure D’s using the SSD / SVT vertex to remove backgroundvertex to remove background

A trigger on high Pt electrons to find B’s through their displaced A trigger on high Pt electrons to find B’s through their displaced vertex.vertex.

Multi-particle correlations using high Pt GammasMulti-particle correlations using high Pt Gammas First steps towards precision measurements of direct GammasFirst steps towards precision measurements of direct Gammas

In addition there were several secondary physics goals which In addition there were several secondary physics goals which include:include:

To measure the upsilon using the L2 triggerTo measure the upsilon using the L2 trigger A ultra-peripheral collision programA ultra-peripheral collision program

These goals are reflected in several specific programs:These goals are reflected in several specific programs:

Revisiting the BUR:Revisiting the BUR:

Page 7: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

Trigger NameTrigger Name Trigger DefinitionTrigger Definition RateRate

MinBias (D’s)MinBias (D’s) ZDC_pre + VPD@5cm + (L2 monitoring)ZDC_pre + VPD@5cm + (L2 monitoring) ~30 hz~30 hz

BHT2-mb (gamma)BHT2-mb (gamma) ZDC + BHT2@~6GeVZDC + BHT2@~6GeV 5 hz5 hz

BHT1-mb (B’s)BHT1-mb (B’s) ZDC + [email protected] + VPD@5cmZDC + [email protected] + VPD@5cm 5 hz5 hz

UpsilonUpsilon ZDC + ZDC + [email protected]@4.5GeV + VPD@30cm + L2 + VPD@30cm + L2 ~40 hz L0/~40 hz L0/

1 hz L21 hz L2

UPCUPC UPC (5<zdcsum<240) (6<ctbsum<200)UPC (5<zdcsum<240) (6<ctbsum<200) 1 hz1 hz

UPC-jpsiUPC-jpsi UPC + JPsiUPC + JPsi 1 hz1 hz

Commissioning Commissioning TriggersTriggers

MuonMuon ZDC + MuonZDC + Muon .1 hz.1 hz

FMSFMS FMSFMS

The requirements for each program were condensed to The requirements for each program were condensed to the following list of triggers before the RHIC run the following list of triggers before the RHIC run began:began:

Page 8: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

In practice, we add triggers to monitor In practice, we add triggers to monitor backgrounds, to help bootstrap luminosities, and backgrounds, to help bootstrap luminosities, and to mark events for priority reconstruction to the to mark events for priority reconstruction to the final running configuration:final running configuration:

The result is a mix of triggers which is optimized The result is a mix of triggers which is optimized and focused towards our physics goals.and focused towards our physics goals.

Page 9: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

Collider Performance:Collider Performance:

The Collider has provided nearly the maximum projected integrated luminosity.The Collider has provided nearly the maximum projected integrated luminosity.

Page 10: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

MM

STAR PerformanceSTAR PerformanceSTAR Data recorded as of June 20th, 8am

87% of 600 ub-1sampled

86% of 75M minbias

Which puts STAR very close to obtaining our minbias and integrated luminosity goals.Which puts STAR very close to obtaining our minbias and integrated luminosity goals.

The integrated luminosity translates to a factor of 20 or more The integrated luminosity translates to a factor of 20 or more increase in statistical significance for rare probes, due to the increase in statistical significance for rare probes, due to the increased acceptance and stability of the EMC, the improved increased acceptance and stability of the EMC, the improved vertex, and increased delivered luminosity.vertex, and increased delivered luminosity.

Page 11: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

STAR TPC image of root(s) = 9.91 GeV AuAu CollisionTaken June 7, 2007.

Run 8158119, Evt 44

RHIC did a one day Low Energy Commissioning Run.RHIC did a one day Low Energy Commissioning Run.

Star commissioned triggers and took a small amount of dataStar commissioned triggers and took a small amount of data

Page 12: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

Run 8158119: (Low Energy Run)- 2288 BBC-small triggers- 403 BBC-large triggers- 214 both BBC small & large- 1 VPD trigger

Page 13: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

Detector UpgradesDetector Upgrades

VPDVPD

DAQ10DAQ10

0000

FMSFMS

MTDMTD

HFTHFT

FWHM ~ 20 cm

The VPD was The VPD was Commissioned during the Commissioned during the first few weeks of the first few weeks of the RHIC run and its RHIC run and its operation was critical to operation was critical to the physics program. the physics program.

Page 14: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

Detector UpgradesDetector Upgrades

VPDVPD

DAQ10DAQ10

0000

FMSFMS

MTDMTD

HFTHFT

In fact, if you superimpose the vertex In fact, if you superimpose the vertex distributions as triggered by the VPD with the distributions as triggered by the VPD with the acceptance for crossing all 3 layers of the SVT, acceptance for crossing all 3 layers of the SVT, the VPD is almost the perfect detector for the the VPD is almost the perfect detector for the job.job.

Page 15: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

Detector UpgradesDetector Upgrades

VPDVPD

DAQ10DAQ10

0000

FMSFMS

MTDMTD

HFTHFT

There is a TPC electronics upgrade to increase the There is a TPC electronics upgrade to increase the maximum TPC event rate to a kilohertz while maximum TPC event rate to a kilohertz while virtually eliminating the deadtime. A single virtually eliminating the deadtime. A single receiver board prototype was installed and is taking receiver board prototype was installed and is taking data. (In red: data from DAQ1000 prototype. data. (In red: data from DAQ1000 prototype. In Black: current TPC)In Black: current TPC)

Page 16: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

Progress On Detector Progress On Detector UpgradesUpgrades

VPDVPD

DAQ10DAQ10

0000

FMSFMS

MTDMTD

HFTHFT

The Forward Meson Spectrometer is a large The Forward Meson Spectrometer is a large extension of the Forward Pion Detector which was extension of the Forward Pion Detector which was commissioned during the gold run and is now ready commissioned during the gold run and is now ready for production running in 2008for production running in 2008

Page 17: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

Progress On Detector Progress On Detector UpgradesUpgrades

VPDVPD

DAQ10DAQ10

0000

FMSFMS

MTDMTD

HFTHFT

2 LMRPC modules From fastoffline trackingAu+Au collisions No track-hit matching yet

The Muon Tracking Detector uses The Muon Tracking Detector uses the metal in the star magnet to the metal in the star magnet to clean up the Muon signal. One clean up the Muon signal. One module was installed and module was installed and incorporated into the STAR trigger incorporated into the STAR trigger during data taking.during data taking.

Page 18: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

Progress On Detector Progress On Detector UpgradesUpgrades

VPDVPD

DAQ10DAQ10

0000

FMSFMS

MTDMTD

HFTHFT

Pixel proto in STAR, measured track density at r = 5cm, z = 145cm

A very small (4mm x 4mm) prototype of the PIXEL A very small (4mm x 4mm) prototype of the PIXEL detector electronics was installed to at r=5cm to detector electronics was installed to at r=5cm to study the background near the beampipe.study the background near the beampipe.

Page 19: 2007 Run Update for STAR

RHIC & AGS User Meeting - 6/21/2007

SummarySummary

STAR is nearing the end of a successful STAR is nearing the end of a successful run.run.

The STAR trigger is strongly focused The STAR trigger is strongly focused towards meeting the collaborations towards meeting the collaborations physics goals.physics goals.

STAR participated in the Low Energy test STAR participated in the Low Energy test run and was able to obtain data.run and was able to obtain data.

There is significant progress installing There is significant progress installing and testing new sub-systems and upgrade and testing new sub-systems and upgrade prototypes. prototypes.