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2008.10.30 Smd emergy for right tail (3 to 30 strips)

Updated on Thu, 2008-10-30 16:39. Originally created by seluzhen on 2008-10-30 16:39.

Figure 1: Case A

2008.10.30 Smd emergy for left tail (-3 to -30 strips)

Updated on Thu, 2008-10-30 16:47. Originally created by seluzhen on 2008-10-30 16:37.

Figure 1: Case A

2008.10.30 Smd energy for 25 central strips

Updated on Thu, 2008-10-30 16:51. Originally created by seluzhen on 2008-10-30 16:35.

Figure 1: Case A

2008.10.30 Smd energy for 5 central strips

Updated on Thu, 2008-10-30 16:33. Originally created by seluzhen on 2008-10-30 16:33.

Figure 1: Case A

2008.10.30 SMD shower shapes: data, raw, and data-driven MC (12 strips)

Updated on Thu, 2008-10-30 16:31. Originally created by seluzhen on 2008-10-30 16:31.

Figure 1: Case A

2008.10.30 SMD shower shapes: data, raw, and data-driven MC (30 strips)

Updated on Thu, 2008-10-30 16:53. Originally created by seluzhen on 2008-10-30 16:27.

Figure 1: Case A

2008.10.30 Various cuts study (pt, Esmd, 8 strips replaced)

Updated on Thu, 2008-10-30 16:46. Originally created by seluzhen on 2008-10-30 16:24.

Ilya Selyuzhenkov October 30, 2008

STAR Management Meeting

Updated on Wed, 2008-10-29 10:56. Originally created by nxu on 2008-10-28 13:53.
2008-10-29 10:00
2008-10-29 11:00
Etc/GMT-7
Wednesday, 29 October 2008
BNL, 50-I-189, at 14:00 (GMT), duration : 01:00

Conference Phone Number: 510 486 7333

   Time:  10 - 11 am EDT

 * --===================================--*

  Agenda:

    0) Requests of captial funds for FY09 - Bill

    1) Requests  of R&D funds for FY09 - Helen/Zhangbu

    2) Run07 issues - Jerome/Bedanga

   3) AOB

* --===================================--*

    Brief Summary:

   1) Will have a special Management meeting to discuss the funding problems, next Monday, 130pm EST.

   2) Next Coll. meeting: in the week of Sept. 14th, Yale or Berkeley / Next analysis meeting: in the week of July 6th, at MIT.

 

Non-photonic electrons in d+Au 2008

Updated on Wed, 2008-10-29 08:46. Originally created by dunlop on 2008-10-28 10:55.

 I decided to take a first look at non-photonic electrons in d+Au 2008, in an attempt to do e-D0 correlations.

Cuts are mostly the default of the previous e-D0 analyses:

Panic Talk on Eta An

Updated on Tue, 2008-10-28 09:17. Originally created by heppel on 2008-10-28 09:17.

This differs from Len's only in the first 4 slides.

Bulk Correlations Physics Working Group EVO meeting

Updated on Wed, 2008-10-29 21:47 by chajecki. Originally created by lisa on 2008-10-28 08:01.
2008-10-29 11:00
2008-10-29 12:30
Etc/GMT-5
Wednesday, 29 October 2008
EVO, STAR Community, at 15:00 (GMT), duration : 01:30
Meeting is locked (you cannot add new talks anymore)

Please upload agenda items, or links to agenda items

S&C Infrastructure Servers

Updated on Mon, 2021-02-01 17:16. Originally created by wbetts on 2008-10-27 18:03.

 

2008.10.27 SMD-based shower shape scaling: 25 strips cluster energy, raw vs. data-driven MC

Updated on Mon, 2008-10-27 15:50. Originally created by seluzhen on 2008-10-27 15:47.

Ilya Selyuzhenkov October 27, 2008

Data sets:

Draft STAR note

Updated on Mon, 2008-10-27 09:45. Originally created by spinka on 2008-10-27 09:45.

Draft STAR note

STAR database inrastructure improvements proposal

Updated on Tue, 2009-05-05 13:45 by testadmin. Originally created by dmitry on 2008-10-25 07:45.

 

STAR database improvements proposal

Comparison of spectra run 3 vs run 8

Updated on Fri, 2008-10-24 15:59. Originally created by dunlop on 2008-10-24 15:59.

 Below is an attempt to look at spectra in run 8 vs run 3 d+Au.

nonphotonic electrons in the Endcap EMC

Updated on Fri, 2008-10-24 03:33. Originally created by subbanly on 2008-10-24 03:33.

nonphotonic electrons in the Endcap EMC

Medium density from IAA

Updated on Mon, 2008-11-03 08:33. Originally created by mvl on 2008-10-23 07:09.

In order to see how well our IAA measurement constrains the medium density in models, I started making a comparison following the method by Jamie Nagle.

STAR Management Meeting

Updated on Wed, 2008-10-22 09:21. Originally created by nxu on 2008-10-20 18:39.
2008-10-22 10:00
2008-10-22 11:00
Etc/GMT-7
Wednesday, 22 October 2008
BNL, 50-I-189, at 14:00 (GMT), duration : 01:00

Conference Phone Number: 510 486 7333

   Time:  10 - 11 am EDT

 * --===================================--*

  Agenda:

    0) Joule targets for FY09 - Bill

    1) QM09 speaker discussions - Nu

    2) STAR computing plan - Jerome

* --===================================--*

    Brief Summary:

    0) Performance Goal for FY09: # of events to be recorded, 4 weeks at 500 GeV p+p collisions, 11 weeks at 200 GeV p+p collisions.

       - 150Hz, 50hr/week, HT/jet patch trigger for W I.D.+M.B., ~120M events for 500 GeV p+p collisions.

       - 400+Hz, 63hr/week,  ~ 900M events for 200 GeV p+p collisions.

         Bernd will discuss this in Spin group for discussions.

2008.10.21 Shower shapes, 5/25 strips cluster energy, raw vs. data-driven MC

Updated on Tue, 2008-10-21 16:09. Originally created by seluzhen on 2008-10-20 17:09.

Ilya Selyuzhenkov October 21, 2008

Data sets: