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HBT

Updated on Thu, 2006-01-05 11:06. Originally created by fretiere on 2006-01-05 11:06.
-00-00
Thursday, 1 January 1970
, at 00:00 (GMT), duration : 00:00
TimeTalkPresenter
17:30 K pi correlations in d+Au and Au+Au ( 00:10 ) 0 filesMikhail Kopytine (Kent State)

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HBT

Updated on Thu, 2006-01-05 11:06. Originally created by fretiere on 2006-01-05 11:06.
-00-00
Thursday, 1 January 1970
, at 00:00 (GMT), duration : 00:00
»

HBT

Updated on Thu, 2006-01-05 11:06. Originally created by fretiere on 2006-01-05 11:06.
-00-00
Thursday, 1 January 1970
, at 00:00 (GMT), duration : 00:00
TimeTalkPresenter
17:30How we construct correlation functions ( 00:10 ) 0 filesMikhail Kopytin (Kent State University)
17:40RQMD vs HBT radii ( 00:10 ) 0 filesFabrice Retiere (TRIUMF)
17:50Identical pi-pi correlations in Au+Au collisions. Source imaging. ( 00:10 ) 0 files
18:00Non-radical clean-up of StHbt ( 00:10 ) 0 filesMike Lisa (OSU)

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HBT

Updated on Thu, 2006-01-05 11:06. Originally created by fretiere on 2006-01-05 11:06.
-00-00
Thursday, 1 January 1970
, at 00:00 (GMT), duration : 00:00
TimeTalkPresenter
07:30bin summing in pi-Xi ( 00:15 ) 0 files

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HBT

Updated on Thu, 2006-01-05 11:06. Originally created by fretiere on 2006-01-05 11:06.
-00-00
Thursday, 1 January 1970
, at 00:00 (GMT), duration : 00:00
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CuCu22 (2005)

Updated on Wed, 2012-12-19 14:45. Originally created by genevb on 2005-12-30 11:40. Under:

Comparison of RICH scalers

The low energy CuCu runs are a difficult spot for E-by-E SpaceCharge calibrations: the time-averaged multiplicity of recorded tracks traversing the TPC is unlikely
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HSI

Updated on Mon, 2007-11-12 20:42 by testadmin. Originally created by jeromel on 2005-12-22 12:46. Under:

This is an highlight of the HSI features. Please, visit the HSI Home Page for more information.
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HTAR

Updated on Thu, 2005-12-22 12:45. Originally created by jeromel on 2005-12-22 12:36. Under:
To use htar within the HPSS environment, users are required to have the valid Kerberos credentials.

The following is the man page of how to use htar. 

   
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HPSS services

Updated on Thu, 2005-12-22 12:28. Originally created by jeromel on 2005-12-22 12:27. Under:

Database opened issues

Updated on Wed, 2005-12-21 11:53. Originally created by testadmin on 2005-12-21 11:52.

Reference

Speaker : Mike DePhillips ( BNL )


Talk time : 12:45, Duration : 00:10

AOB

Updated on Wed, 2005-12-21 11:52. Originally created by testadmin on 2005-12-21 11:41.

Reference

Speaker : All


Talk time : 12:55, Duration : 00:05

Herwig news

Updated on Wed, 2005-12-21 11:41. Originally created by testadmin on 2005-12-21 11:40.

Reference

Speaker : Maxim Potekhin ( BNL )


Talk time : 12:35, Duration : 00:10

Feedback on production removal

Updated on Wed, 2005-12-21 11:40. Originally created by testadmin on 2005-12-21 11:38.

Reference

Speaker : All


Talk time : 12:25, Duration : 00:10

Kalman modifications in Sti

Updated on Wed, 2005-12-21 11:38. Originally created by testadmin on 2005-12-21 11:35.

Reference

Speaker : Victor Perevoztchikov ( BNL )


Talk time : 12:15, Duration : 00:10

SVT alignement progress report

Updated on Wed, 2005-12-21 11:35. Originally created by testadmin on 2005-12-21 11:34.

Reference

Speaker : Spiros Margetis ( KSU )


Talk time : 12:00, Duration : 00:15

Imaging C(q_inv)

Updated on Wed, 2005-12-21 10:15. Originally created by bystersky on 2005-12-21 10:12.

Reference

Speaker : MIchal Bystersky


Talk time : 17:40, Duration : 00:10

http://www.star.bnl.gov/protected/hbt/bystersk/meeting/2005_12_21/imaging.pdf

Comparing K-pi correlations in d+Au with HIJING

Updated on Tue, 2005-12-20 18:45. Originally created by kopytin on 2005-12-20 18:45.

Reference

Speaker : Mikhail Kopytine ( Kent State University )


Talk time : 17:30, Duration : 00:10

replacement

Updated on Tue, 2005-12-20 14:10. Originally created by ullrich on 2005-12-20 14:10.

Reference


Talk time : 14:40, Duration : 00:10

Update on 62GeV

Updated on Tue, 2005-12-20 14:04. Originally created by bielcik on 2005-12-20 12:31.

Reference

Speaker : A.Knospe ( Yale )


Talk time : 14:30, Duration : 00:10

Anders made AuAu200/AuAu62 plot to see how much yield we claim to reconstruct
compare how much we expect from cross sections

http://www.star.bnl.gov/protected/heavy/bielcik/aknospe/AuAu62_2012_200

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Ian Johnson's way to calculate the invariant mass

Updated on Tue, 2005-12-20 10:48. Originally created by ullrich on 2005-12-20 10:48.

Reference

Speaker : Weijiang Dong


Talk time : 13:20, Duration : 00:10

I used Ian Johnson's way to calculate the invariant mass. I also applied a
few opening angle cuts and tightened two-track-DCA cut.
The final electron v2's statistical error can be reduced by this method!