Difference between revisions of "CommonNtuple"

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   data10_7TeV.00155678.physics_MuonswBeam.recon.ESD.f261
 
   data10_7TeV.00155678.physics_MuonswBeam.recon.ESD.f261
 
   data10_7TeV.00155697.physics_MuonswBeam.recon.ESD.f261
 
   data10_7TeV.00155697.physics_MuonswBeam.recon.ESD.f261
 +
 +
monte carlo at nikpc10:
 +
  /data/sandstro/NTUP/MC/
  
 
short (PERSONAL) recipe how I got thing to work at lxplus:
 
short (PERSONAL) recipe how I got thing to work at lxplus:

Revision as of 12:31, 9 June 2010

code:

  https://svnweb.cern.ch/trac/atlasusr/browser/sandstro/CommonNtuple
  contains MuonESDAnalysis and MCPAnalysis

ntuples (output of MuonESDAnalysis):

  at nikhef: /data/atlas2/users/egge/MuonESDAnalysis/MuonswBeam/

used datasets (status 9 June 2010):

  data10_7TeV.00153565.physics_MuonswBeam.recon.ESD.r1297/
  data10_7TeV.00153599.physics_MuonswBeam.recon.ESD.r1297/
  data10_7TeV.00154810.physics_MuonswBeam.recon.ESD.r1297/
  data10_7TeV.00154813.physics_MuonswBeam.recon.ESD.r1297/
  data10_7TeV.00154815.physics_MuonswBeam.recon.ESD.r1297/
  data10_7TeV.00154817.physics_MuonswBeam.recon.ESD.r1297/
  data10_7TeV.00154822.physics_MuonswBeam.recon.ESD.r1299/
  data10_7TeV.00155073.physics_MuonswBeam.recon.ESD.r1299/
  data10_7TeV.00155112.physics_MuonswBeam.recon.ESD.r1299/
  data10_7TeV.00155116.physics_MuonswBeam.recon.ESD.r1299/
  data10_7TeV.00155160.physics_MuonswBeam.recon.ESD.r1299/
  data10_7TeV.00155228.physics_MuonswBeam.recon.ESD.f259
  data10_7TeV.00155280.physics_MuonswBeam.recon.ESD.f259
  data10_7TeV.00155569.physics_MuonswBeam.recon.ESD.f260
  data10_7TeV.00155634.physics_MuonswBeam.recon.ESD.f260
  data10_7TeV.00155669.physics_MuonswBeam.recon.ESD.f260
  data10_7TeV.00155678.physics_MuonswBeam.recon.ESD.f261
  data10_7TeV.00155697.physics_MuonswBeam.recon.ESD.f261

monte carlo at nikpc10:

  /data/sandstro/NTUP/MC/

short (PERSONAL) recipe how I got thing to work at lxplus:

  /afs/cern.ch/user/e/egge/public/instructionsMuonESDAnalysis.txt

Production is done on lxplus batch, using FileStager to retrieve ESD's from Grid. An example of a batch job I run for production:

  #!/bin/zsh
  source /afs/cern.ch/atlas/project/muon/software/egge/15.6.9.13/setup.sh -tag=15.6.9.13,AtlasProduction
  source /afs/cern.ch/user/e/egge/grid.sh
  cp /afs/cern.ch/user/e/egge/public/MuonESDAnalysis/readesdGrid.py .
  cp /afs/cern.ch/user/e/egge/public/MuonESDAnalysis/an.py .
  cp -r /afs/cern.ch/user/e/egge/public/MuonESDAnalysis/samples/ .
  cp /afs/cern.ch/user/e/egge/public/MuonESDAnalysis/input_FileStager.py .
  cp /afs/cern.ch/user/e/egge/public/MuonESDAnalysis/configureServices.py .
  ln -s samples/0155116_0.def sample.def
  athena -s readesdGrid.py >! log.l &

Action Items:

  Just as a summary, here are the action items from our meeting. I tried to put the names of the responsible person next to it:
  1) Check that all the variables are in Egge's Ntuples:
     a) truth info (Michele->Egge)
     b) Alan's variables (Giuseppe->Egge)
  2) Check that all the needed MC/data is produced (all)
     If you're missing something, send an email to Egge stating the dq2 sample name and he will start if for you.
  3) For may-reprocessing data check that all the right LB's are used as given by MCP   (Alex)
  4) Ks->pi pi to validate the templates for decays-in-flight (Alex)
  5) MEETING FRIDAY 11 june at 10:00 (ALL)
     see Giuseppe's email for details
  ps. I understand that there were many more requests and action-items, but agreeing with Michele I do no think that it is feasible to finish all of that before friday/monday-tuesday MCP meetings, but feel free to add items to my list.