STAR Protected

HFT Face to Face

2012-05-18 09:00
America/New York
Friday, 18 May 2012
BNL, at 13:00 (GMT), duration : 00:00

Regular HFT technical and management meeting. Final notification on meeting room at BNL will be send out and updated here.

The EVO information is:

Title:                HFT f2fB

Description:     Regular tc face to face meeting

Community:     STAR

Password:       star

 

Meeting Access Information:

- Meeting URL

            http://evo.caltech.edu/evoNext/koala.jnlp?meeting=MsMiMI2s2IDBD99B9vDt9s

 

- Password: star

- Phone Bridge

            ID: 526 3442

            Password: 0952

TimeTalkPresenter
09:00HFT overview ( 00:20 ) 1 fileF Videbaek
09:30Schedule&Cost ( 00:30 ) 1 fileS.Morgan
10:00Global Structure, Assembly ( 00:30 ) 1 fileE.Anderssen
10:30break ( 00:20 ) 0 files
10:50Integration ( 00:20 ) 1 fileR.Sharma
11:10IST status ( 00:30 ) 1 fileGerrit J. van Nieuwenhuizen II (Massachusetts Institute of Technology)
11:40PXL Mechanical ( 00:15 ) 2 filesH.Wieman
11:55SSD overview ( 00:20 ) 1 fileJim Thomas
12:15Lunch ( 01:15 ) 0 files
13:30CMM review closeout ( 00:30 ) 1 file
14:00PXL electric ( 00:20 ) 1 fileL.Greiner
14:20SSD electronics Upgrade ( 00:20 ) 1 fileM. LeVine
14:40HFT Software ( 00:20 ) 1 fileS.Margetis
15:30Summary discussion ( 01:20 ) 0 filesAll

Summary and Discussion

Break

MTD muon PID

Speaker : Bingchu Huang (presented by W.J. Llope)


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

TOF Calibrations

electron PID

TOF & dE/dx PID and resolution

Using the calorimeters in MuDsts for e,gamma,jets

Break

Using the SMDs for gamma and pi-zero

Photons and Neutral Pions in the STAR Forward Meson Spectrometer

Event by event di-hadron correlations in heavy-ion collisions

Higher Moments of Net-proton Multiplicity Distributions from RHIC Beam Energy Scan

Speaker : Xiaofeng Luo ( CCNU )


Talk time : 11:00, Duration : 00:45

Net-proton C6/C2

Break

moments

Higher Moments of Net Particle Numbers

Net-charge moments

Particle Ratio Fluctuation Results and Properties of the Observable, $\nu_{dyn}

Break