Difference between revisions of "AtlasTopPhysicsSamples"
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| style ="background:#3399ff;" | Sample | | style ="background:#3399ff;" | Sample | ||
| + | | style ="background:#3399ff;" | Sub-sample | ||
| style ="background:#3399ff;" | Location | | style ="background:#3399ff;" | Location | ||
| style ="background:#3399ff;" | Statistics | | style ="background:#3399ff;" | Statistics | ||
|- | |- | ||
| − | | AOD | + | | AOD |
| − | | [http://www.nikhef.nl/pub/experiments/atlas/public/Rome/A7/AOD/ Repository] | + | | Rome |
| + | | [http://www.nikhef.nl/pub/experiments/atlas/public/Rome/A7/AOD/AOD_Rome Repository] | ||
| ~4000 files of 50 events | | ~4000 files of 50 events | ||
|- | |- | ||
|} | |} | ||
Revision as of 10:29, 12 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: events using MCatNLO. Fully hadronic events have been rejected.
T2: events using MCatNLO. Fully hadronic events have been rejected and 1 top has 500 GeV
A7: W+4jet events using AlpGen.
Links to the various files ?
| T1 sample |
|---|
| Sample | Sub-sample | Location | Statistics |
| MatrixElement files | Repository | 200 files of 12,500 events | |
| Generator POOL files | Repository | 200 files of 5,000 events | |
| CBNT | Rome | Repository | ~6000 files of 50 events (1000 missing) |
| AOD | AtlFast | Repository | 200 files of 5000 events |
| Rome | Repository | ~4000 files of 50 events | |
| New | Repository | ~1000 files of 50 events (6000 missing) |
| T2 sample |
|---|
| Sample | Sub-sample | Location | Statistics |
| MatrixElement files | Repository | 100 files of 12,500 events | |
| Generator POOL files | Repository | 100 files of 5,000 events | |
| CBNT | Rome | Repository | 100 files of 50 events |
| AOD | Not available | None |
| A7 sample |
|---|
| Sample | Sub-sample | Location | Statistics |
| AOD | Rome | Repository | ~4000 files of 50 events |