BEMC (EEMC) tower data simulation comparison

Tower threshold 250MeV.

TOF OPS: How to mask TOF trays in/out of the L0 tofmult trigger

ssh staruser@startrg

cat README.TofMaskProgram

find the latest tof.[timestamp].dat file: ls -lrst tof.*.dat

copy it to a new file with a new timestamp.

Quick look at fitting stability using W triggers in run 11

This obviously needs some explaining: the colors corresponding to the nofixedparam are full fits (i.e., gaussian peak for pion, exponential background with a curvature term in it and a gaussian to

IPHC phone conference report

Speaker : Leo Greiner


Talk time : 09:00, Duration : 00:20

STAR BUR Run 12/13

Repeat Rehearsal Talk - di-electron measurements

Repeat Rehearsal Talk - LPV

BES talk

Speaker : Bedanga Mohanty ( VECC )


Talk time : 15:00, Duration : 00:30

Repeat Rehearsal Talk - Highlights from STAR

STAR as a fixed target experiment

Speaker : Daniel Cebra ( UC Davis )


Talk time : 12:00, Duration : 00:30

New results from Spin PWG

Speaker : Carl Gagliardi part deux!


Talk time : 11:00, Duration : 01:00

Sector dependent SMD breakout in the EEMC

Sector dependent shower shape distributions

(I)Sectors 1, 4, 7 and 10 have the same structure of V, Space and U.

Run9 Nsigma vs beta Fit Result for E and Pi

This is a fit result for run 9 tof data.

For pion, the fits are valid up to around p = 1.2 GeV/c.

For electron, the fits are valid up to around p = 0.4 GeV/c.

Shower Shape Distributions (Normalized w.r.t center strip)

Shower Shape Distributions

These three curves have been normalized w.r.t center strip.

AOB


Talk time : 12:40, Duration : 00:20

Residuals in ideal TPC alignment simulations

Speaker : G. Van Buren ( BNL )


Talk time : 12:20, Duration : 00:20

 See here.

Run 11 Calibrations update

Speaker : G. Webb ( UKy )


Talk time : 12:00, Duration : 00:20

 Here is the work done on the initial dE/dx calibration for Run 11 pp500GeV.

Software and Computing Meeting

2011-05-11 12:00
2011-05-11 13:00
America/New York
Wednesday, 11 May 2011
1-189, EVO, at 16:00 (GMT), duration : 01:00
TimeTalkPresenter
12:00Run 11 Calibrations update ( 00:20 ) 2 filesG. Webb (UKy)
12:20Residuals in ideal TPC alignment simulations ( 00:20 ) 0 filesG. Van Buren (BNL)
12:40AOB ( 00:20 ) 0 files

single D0's with long ctau

For some studies, I have generated with starsim 10k D0's (1D0 per event) with power law pt (in 0<pT<5) but with a larger timelife :

Shower shape distributions (Comparison with MC)

Photon Candidate Transverse Shower Profile Distributions

u plane