Proton-lambda residual correlations in proton-proton- update
Updated on Wed, 2005-10-26 11:32. Originally created by hbtuser on 2005-10-26 11:32.Reference
Speaker : Hania Gos ( Warsaw University of Technology, SUBATECH )
Talk time : 19:00, Duration : 00:10
GL_pp400_X30_High
Updated on Wed, 2005-10-26 10:42. Originally created by genevb on 2005-10-26 10:42.
GridLeak plot for pp400 data with 30% above standard pp200 corrections, high luminosities
GL_pp400_X17_Lowest
Updated on Wed, 2005-10-26 10:41. Originally created by genevb on 2005-10-26 10:41.
GridLeak plot for pp400 data with standard pp200 corrections, lowest luminosities
GL_pp400_X17_High
Updated on Wed, 2005-10-26 10:41. Originally created by genevb on 2005-10-26 10:40.
GridLeak plot for pp400 data with calibrated corrections, high luminosities
GL_pp400_STD_High
Updated on Wed, 2005-10-26 10:39. Originally created by genevb on 2005-10-26 10:37.
GridLeak plot for pp400 data with standard pp200 corrections, high luminosities
GL_pp400_NONE_Low
Updated on Wed, 2005-10-26 10:35. Originally created by genevb on 2005-10-26 10:34.GL_pp400_NONE_High
Updated on Wed, 2005-10-26 10:34. Originally created by genevb on 2005-10-26 10:33.
GridLeak plot for pp400 data with no correction, high luminosities
AOB
Updated on Wed, 2005-10-26 10:58. Originally created by testadmin on 2005-10-26 10:30.GridLeak plots
Updated on Thu, 2005-11-17 14:42. Originally created by genevb on 2005-10-26 10:28. Looking at the residuals (GridLeak plots), I can see that things are similar to pp200, witth what appears to be an offset in GridLeak distortion at all z (our current understanding of the distortion has it go to zero at the ground planes, |z| = 208 cm). I include here three plots of GridLeak distortion residuals from tracks for high luminosity pp400 data (runs 6154024-6154031, bbce+bbcw > 2e5):
Production update
Updated on Wed, 2005-10-26 09:55. Originally created by testadmin on 2005-10-26 09:54.MC comparison TPT/ITTF for Au+Au and Cu+Cu
Updated on Wed, 2005-10-26 09:53. Originally created by testadmin on 2005-10-26 09:50.STAR Upgrades Meeting
Updated on Wed, 2005-10-26 09:50. Originally created by dunlop on 2005-10-26 09:49. -00-00
from Thursday, 1 January 1970 to Thursday, 1 January 1970
Conference duration: 1 day
Upgrades meeting
»
Calibration status for Cu+Cu and p+p 400 GeV
Updated on Wed, 2005-10-26 11:22. Originally created by testadmin on 2005-10-26 09:48.Reference
Speaker : Gene Van Buren ( BNL )
Talk time : 12:00, Duration : 00:15
December 2005 STAR Analysis Meeting
Updated on Wed, 2005-10-26 09:40. Originally created by dunlop on 2005-10-26 09:38. -00-00
from Thursday, 1 January 1970 to Thursday, 1 January 1970
Conference duration: 1 day
Biannual STAR Analysis Meeting
»
SHD in CUCU200
Updated on Wed, 2005-10-26 01:39. Originally created by hbtuser on 2005-10-26 01:39.WPCF proceedings (pi-Xi)
Updated on Tue, 2005-10-25 23:31. Originally created by chajecki on 2005-10-25 23:30.Reference
Speaker : Petr Chaloupka
Talk time : 18:40, Duration : 00:10
http://www.star.bnl.gov/protected/hbt/petrchal/talk/proc/wpcf.pdf
WPCF proceedings
Updated on Tue, 2005-10-25 22:01. Originally created by chajecki on 2005-10-25 22:00.Reference
Speaker : Zbigniew Chajecki ( OSU )
Talk time : 18:30, Duration : 00:10
http://www.star.bnl.gov/protected/hbt/chajecki/proceedings/WPCF2005/
GL_pp400_NONE_Low
Updated on Tue, 2005-10-25 18:59. Originally created by genevb on 2005-10-25 18:58.
GridLeak plot for pp400 data with No corrections, low-range luminosities
GL_pp400_NONE_Mid
Updated on Tue, 2005-10-25 18:57. Originally created by genevb on 2005-10-25 18:55.
GridLeak plot for pp400 with No correction, mid-range luminosities.
Analysis meeting
Updated on Tue, 2005-10-25 18:54. Originally created by fretiere on 2005-10-25 18:52.Reference
Talk time : 18:20, Duration : 00:10
Are you planning to come to the Collaboration meeting?