Difference between revisions of "AtlasTopPhysicsSamples"
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| Line 31: | Line 31: | ||
|rowspan=4 valign="center" align = "center"| T1 | |rowspan=4 valign="center" align = "center"| T1 | ||
| MatrixElement file | | MatrixElement file | ||
| − | | http://www.nikhef.nl/ | + | | http://www.nikhef.nl/pub/experiments/atlas/public/Rome/T1/MatrixElement/ |
| 200 files of 12,500 events | | 200 files of 12,500 events | ||
|- | |- | ||
Revision as of 12:04, 11 September 2005
Location of ATLAS top group physics samples
The information below is NOT yet accurate
What are the different samples ?
A short description of the sample necessary for the Rome tt analysis:
T1: tt events. Fully hadronic events have been rejected.
T2: tt events. Fully hadronic events have been rejected and at least one of the tops has a greater than 500 GeV/c
A7: (W + 4 jets)-events. The dominant background for the tt analysis.
Links to the various files ?
| Sample | Type | Location | Statistics |
| T1 | MatrixElement file | http://www.nikhef.nl/pub/experiments/atlas/public/Rome/T1/MatrixElement/ | 200 files of 12,500 events |
| POOL & CBNT files | /project/atlas/users/ivov/Rome_project/MCatNLO/POOLCBNT/ | 200 files of 5,000 events | |
| AOD files | /project/atlas/users/verkerke/RomeData/recov10/4100/ | 4000 files of 50 events | |
| AOD from ATLFAST | /project/atlas/users/mlimper/FAST_AOD/t1/ | 200 files of 5,000 events |