Editing Luter Plots (section)

==Overview==

Luter Plots has many iterations where each is an analysis script that gives around 10 cool plots. This page specifically covers the [https://en.wikipedia.org/wiki/Project_Jupyter#Jupyter_Notebook Jupyter Notebook] version we made. 

rdfluterplots is a jupyter notebook that takes a <code>.root</code> file containing [[Cosmic_Ray_Detection_(Losada,_Freeman,_Lyon,_Trant)|cosmic ray data]], analyzes the data using [https://root.cern/doc/master/classROOT_1_1RDataFrame.html RDataFrame], and displays them using [https://en.wikipedia.org/wiki/CERN CERN]'s [https://en.wikipedia.org/wiki/ROOT ROOT] framework.

===Script Usage===

The Jupyter Notebook is located at this link: [http://jlabdaq.pcs.cnu.edu:8000/user/jlabdaq/lab/tree/analyzer/rdfluterplots.ipynb rdfluterplots]

===Input Run===
Data for different runs is stored in root files label with the run number. For example, run 40 is saved to the file <code>rootfiles/test40.root</code>. So, by changing the <code>filename</code> variable in cell 2, you can select the run data you want to analyze.

===Changing Functions===
The program defines all of its functions in C++ and uses [https://root.cern.ch/doc/master/classTInterpreter.html ROOT gInterpreter] to make the C++ code accessible to the rest of the python script. These functions are mostly found in the third cell. Everything inside this <code>trigger</code> comment block must be written in C++ format.