The STAR experiment

Time	Talk	Presenter
13:00	SVT hardware status ( 00:15 ) 2 files	David Lynn (BNL)
13:15	Strange Physics with and without the SVT ( 00:20 ) 3 files	Helen Caines (Yale)
13:35	SVT, an active pile-up rejector ( 00:20 ) 0 files	Spiros Margetis (KSU)
13:55	Topological reconstruction of D0 decays ( 00:25 ) 1 file	Sarah LaPointe (WSU)
14:20	D-meson mixed event analysis ( 00:20 ) 3 files	Christina Markert (KSU)
14:40	B-Meson reconstruction with the SVT ( 00:20 ) 3 files	Mark Heinz (Yale)
15:00	Using the SVT for rejection of photon conversion ( 00:20 ) 3 files	Frank Laue (BNL)

Time	Talk	Presenter
10:50	Overview of progress and current status of the SVT/SSD tracking effort ( 00:20 ) 4 files	Spiros Margetis (KSU)
11:10	The use of Silicon detectors for future TPC Calibration ( 00:20 ) 2 files	Gene Van Buren (BNL)
11:30	SVT calibration issues and remaining tasks for the future ( 00:15 ) 3 files	Yuri Fisyak (BNL)
11:45	Self-alignment status and perspectives ( 00:15 ) 2 files	Victor Perevoztchikov (BNL)

Email from Tim Hallman, Spokesman for STAR sent on 5/27/2006 14:50

Dear STAR Collaborators,

The email concerns an upcoming planning exercise related to
STAR's inner tracking detectors. The review, which will take place
 
Reference
Event : STAR Inner Silicon tracking detector review
Session : Introduction
Timetable : detailed

 Talk time : 08:45, Duration : 00:15

Time	Talk	Presenter
08:45	Welcome ( 00:15 ) 0 files
09:00	Overview of STAR's BUR and main physics goals for the near term future ( 00:30 ) 1 file	James Dunlop (BNL)
09:30	R&D time constraints, the HFT perspectives ( 00:15 ) 2 files	Jim Thomas (LBNL)
09:45	SVT removal, the engineering perspective ( 00:15 ) 1 file	Ralph Brown (BNL)
10:00	Spin PWG Perspectives ( 00:15 ) 2 files	Scott Wissink (IUCF)
10:15	Benefit of the removal of the SVT for e- measurement ( 00:20 ) 2 files	Thomas Ullrich (BNL)

- Charges and review annoucements are available in the You do not have access to view this node link.
Members of the review panel

• Tim Hallman (Chair)
• Jack Sandweiss
• Tom Ludlam
• Howard Wieman
• Steve Vigdor

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The method of determining the amount of SpaceCharge present in the TPC from the sDCA of global tracks has worked well in the productions where only TPC hits have been used on tracks.

Mean of sDCA distirbutions are hollow markers; gaussian width of sDCA distributions are solid markers. P06ib data is black, P06ic data is red, and day 40 data for P06ib and P06ic are in green and blue respectively.