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Updated on Tue, 2012-10-16 00:10 by sichterm. Originally created by xzb on 2012-10-16 00:10.
2012-10-16 12:00
2012-10-16 13:00
America/New York
Tuesday, 16 October 2012
EVO 14 3853 (Tuesday 10/02 noon), at 16:00 (GMT), duration : 01:00
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An estimation of neutron flux in STAR WAH (first round)

Updated on Tue, 2012-10-16 14:34. Originally created by fisyak on 2012-10-15 19:13.

I have made a priliminary estimation of neutron flux in WAH based on existing geometry for WAH (Jason), and geant/gcalor version with low kinematical cuts (electons, gamma = 10 keV,

FCS Simulation

Updated on Sun, 2012-12-02 14:33. Originally created by leun on 2012-10-15 18:08.

 

2006 EEMC Neutral Pions: Transverse Single-spin Asymmetry (First Look)

Updated on Thu, 2012-10-18 15:37. Originally created by drach09 on 2012-10-15 16:38.

Much work has been devoted to improving and building upon the 2006 EEMC π0 longitudinal analysis.

How useful do you think EVO is for our community and Video Tele Conferencing?

Updated on Mon, 2012-11-05 11:12 by testadmin. Originally created by jeromel on 2012-10-15 13:36.

* Extremely important, cannot imagine our community without it
* Important, I use it often and rely on it to join/organize meetings frequently
* Somewhat important, I use it sometimes but also use other tools
* Not that important, I use other tools or phone bridge for our STAR use
* Not important at all, the tool is bad and I don't understand why we use it in STAR
* I have no opinion

DNP Meeting Talk

Updated on Wed, 2012-10-24 09:39. Originally created by sdhamija on 2012-10-15 12:56.

 

FMS DB entries for LED and pi0 mass corrections part 2

Updated on Mon, 2012-10-15 13:25. Originally created by tpb on 2012-10-15 09:14.

There were discussions a couple of weeks ago regarding how best to implement our LED correction scheme in the database.

DNP2012-draft1

Updated on Sun, 2012-10-14 16:20. Originally created by plyku114 on 2012-10-14 16:20.

2nd round of comments on Tlusty's proceeding

Updated on Sat, 2012-10-13 19:43. Originally created by weixie on 2012-10-13 19:43.

QCD-N Talk Len Eun

Updated on Tue, 2013-02-19 16:45. Originally created by leun on 2012-10-13 18:24.

 

DNP 2012 Talk

Updated on Thu, 2012-10-18 12:59. Originally created by sgliske on 2012-10-13 16:20.

Version 1 last updated Saturday, Oct 13th, at 4:20 PM CST.

Version 2 last updated Tuesday, Oct 16th, at 5:00 PM CST.

FMS-EEMC update 20121012

Updated on Sat, 2012-10-13 11:14. Originally created by xuanli on 2012-10-13 11:14.

Eemc pi0 Cross Section -- Oct 12 Update

Updated on Fri, 2012-10-12 17:33. Originally created by sgliske on 2012-10-12 16:04.

Here's the updated cross section with the L2 thresholds raised to 10% above max hardware settings (3.9 GeV and 5.5 GeV).  About 100 runs were used, or about 1/3 of the 2nd longitudinal da

DNP 2012 Talk

Updated on Thu, 2012-10-25 20:33. Originally created by pagebs on 2012-10-12 15:58.

max ET vs pi0 pT

Updated on Fri, 2013-01-11 13:41. Originally created by sgliske on 2012-10-12 15:34.

As requested during the SPIN meeting yesterday, I've divided my max tower ET plots into reconstructed pi0 pT bins.  I've also included the max ET (tower) / ET (3x3) plot (with E

Kayla Kutz's poster for the DNP 2012

Updated on Fri, 2012-10-12 14:49. Originally created by tdss on 2012-10-12 14:49.

more comments on Mustafa's QM12 proceeding

Updated on Fri, 2012-10-12 14:22. Originally created by weixie on 2012-10-12 14:22.

AOB

Updated on Fri, 2012-10-12 11:35. Originally created by jeromel on 2012-10-12 11:35.

Reference

Speaker : All


Talk time : 14:50, Duration : 00:10

ESL

Updated on Fri, 2012-10-12 11:55 by lbhajdu. Originally created by jeromel on 2012-10-12 11:34.

Reference

Speaker : Leve


Talk time : 14:40, Duration : 00:10

Calibration and production

Updated on Fri, 2012-10-12 12:45 by genevb. Originally created by jeromel on 2012-10-12 11:34.

Reference

Speaker : Gene, Lidia


Talk time : 14:20, Duration : 00:20

CALIBRATIONS (GENE): 

Automated caibrations:

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