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Cosmic rays study, version 2
This is the result of work I am doing with Amal Sarkar, and is an update of my Initial look at cosmic ray resolutions.
FMS simulation (cont.)
Fig. 1. Reconstructed pi0 mass.
Fig. 2. Photon energy resoluation.
Step One Status Update
We have been able to map out and run most of the frist step(smd slope fitting) of the EEMC calibration. In this step we have identified three sub steps:
Grouped Run Data/Charts for EEMC Calibration
Update: I created graphs for comparing the 6th group to the 3rd group and the 3rd group to the 1st group. I also corrected the titles on the first graphs. Most of the l
STAR Management Meeting
BNL, 50-I-189, at 15:00 (GMT), duration : 01:00
EVO: Title: STAR Management Meeting // Community: STAR // Password: star
Phone Bridge: +1 626 395 2112 (CA) / +1 631 344 6100 (NY) // ID: 56533 // Password: 0952
Time: 11 AM - 12 PM EDT
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I. Agenda:
1) Run 10 Data production - Gene/Jerome/Bedanaga
2) Rotation of co-conveners - Nu
3) Operational review, June 22 version: (1) ppt file; (2) pdf file
4) TBD
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II. Brief Summary and/or Action Items:
1) Attendency:
III. Note:
► Charge for New Decadal Plan, Steve Vigdor, Dec. 17, 2009
► STAR NPE Committee, H. Huang (chair), April 2008
► STAR FMS Review: Sept. 1-2, BNL. P. Jacobs (chair). Review Report
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IV. Future Meetings and Reviews:
► RHIC PAC Meeting: June 21-23, 2010, BNL
► RHIC Science and Technology Review: June 28-30, 2010, BNL
► Spin2010: Sept. 27 - Oct. 2, 2010, Juelich, Germany
► STAR Collaboration Meeting: Oct. 27 - Nov. 1, 2010, BNL. Chair: J. Dunlop
► DNP2010: Nov. 3-6, 2010, Santa Fe, NM
STAR Management Meeting
BNL, 50-I-189, at 15:00 (GMT), duration : 01:00
1) Brief note on the Management - Convener discussions:
Date: 12 noon - 2:20pm, June 16, 2010
Participants: Olga, Jerome, Jamie, Lijuan, Fuqiang, Flemming, Ernst, Paul, Joern, Lanny, Gang, Nu
Note: pdf file
Brief Introduction to the VPD and the TOF Start-side
Updated on Thu, 2010-06-17 20:56 by llope. Originally created by geurts on 2010-06-15 22:16.Reference
Speaker : W.J. Llope
Talk time : 17:00, Duration : 00:20
Initial look at cosmic ray resolutions
This is the result of work I am doing with Amal Sarkar.
Steps:
Smd Iteration Results
Using the first step in the EEMC calibration, fitting the slopes of the smd, we have recived our first results.