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...
How To Guides Below are a list of how to guides that may be useful for you. HowToRunDaVinciAtRAL HowToRunDaVinciOnTheGrid HowToMergeRootFiles HowToCompileRootMacr...