Searched: ^H
Results from LHCb web retrieved at 08:40 (GMT)
Results from LHCb web retrieved at 08:40 (GMT)
How to Calculate Luminosity Creating the ntuple You will need to make sure that the luminosity data is in the ntuple. To do this ckeck that there is a GetIntergratedLuminosity...
How to compile root Macros Why compile with g and not CINT? CINT, the root interpreter, is dead slow and I have seen a very noticeable decrease in the execution...
How to Find A Stripping Line Script There is a script which outputs all of the locations of the various stripping lines in a dst file. The following will print all...
How Merge root files Ganga The easiest way is to let ganga handle it with with the RootMerger() j Job(t) j.merger RootMerger() j.merger.files `out file.root...
How to run DaVinci at RAL Creating an ntuple Real Data to create an ntuple with real data you need the DST files you wish to run on a python file pointing...
How to run DaVinci on the Grid Reconsider First off please reconsider, the ppd batch system works a lot more seamlessly. If you can, use it. GridTips might be a useful...
PIDCalib Package About The Package This package enables the user to properly calibrate the DLL distributions of their signal mode, and thus calculate the efficiency...
EdmundSmith 2010 12 09 B2D0Kst D2Kpi.py.txt: DST writing script.
How To Guides Below are a list of how to guides that may be useful for you. HowToRunDaVinciAtRAL HowToRunDaVinciOnTheGrid HowToMergeRootFiles HowToCompileRootMacr...
Number of topics: 9
Topic revision: r6 - 2010-11-05 - StefaniaRicciardi
Site map
Atlas web
Create New Topic
Index
Search
Changes
Notifications
RSS Feed
Statistics
Preferences
Account 
Copyright © 2008-2024 by the contributing authors. All material on this collaboration platform is the property of the contributing authors. Ideas, requests, problems regarding TWiki? Send feedback