Difference between revisions of "NIKHEF Rome MCatNLO Samples"

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Latest revision as of 09:46, 15 June 2005

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.

Where are the different files located at NIKHEF ?

Sample Type Location Statistics
T1 Event file /project/atlas/users/ivov/Rome_project/MCatNLO/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
T2 Event file /project/atlas/users/ivov/Rome_project/MCatNLO_Pt500/MatrixElement/ 100 files of 12,500 events
POOL & CBNT files /project/atlas/users/ivov/Rome_project/MCatNLO_Pt500/POOLCBNT/ 100 files of 5,000 events
AOD files (empty) (empty)
AOD from ATLFAST /project/atlas/users/mlimper/FAST_AOD/t2/ 100 files of 5,000 events
A7 Event file -- not generated at NIKHEF -- (empty)
POOL & CBNT files -- not generated at NIKHEF -- (empty)
AOD files /project/atlas/users/ivov/Rome_project/WPlus4Jets/AOD/ 3718 files of 50 events

Access to the input- and log-files

Some links to the output- as well as the input-, joboptions- and log-files can be found here:

T1 sample (4100)

  1. producing the event-files
  2. running the event files through Herwig

T2 sample (4101)

  1. producing the event-files
    • Event files (For each job 1 files: event file)
    • These files were filtered from a large set of normal tt event-files
  2. running the event files through Herwig