Now that we have finished with the ntuple production steps, we will shift focus to doing some common analysis procedures on ntuples. The next few sections will focus on building an analysis from ntuples, but first let’s look at the ntuples that you have produced and the centrally-produced ntuples that you will use in the next steps.
In the AnaAlgorithm steps up to this point, you have been running over a single ttbar sample and have added a small number of branches that hold information about a few physics object collections as well as missing transverse energy.
You can check the ntuple content by opening (from the run
directory) submitDir/data-ANALYSIS/dataset.root
and using
a TBrowser
. The analysis
tree should have the following
branches:
As a reminder, the el_*
, mu_*
and jet_*
branches are
vectors of float
corresponding to physics objects in each
event while the met_*
branches are float
and runNumber
and eventNumber
are int
since one value exists for each
event.
A single simulated ttbar background sample is not sufficient to perform a physics analysis and the set of information contained in your ntuple is very limited. Rather than having you extend the ntuple content and go through the time consuming step of running your code over several dozen samples, complete ntuples produced from the necessary samples are provided.
The full set of provided ntuples are available at /eos/user/j/jveatch/tutorial/ntuple/
.
The available samples are split into the following directories:
signal
: numerous leptoquark signal samples with varying
masses, widths, and other model parametersdata
: a subset of the available ATLAS Run 2 detector datattbar
, wjets
, etc.: the complete set of each background
process that is important for the analysisWithin each directory, you will see files named *_out.root
.
For the signal and background samples, the six digit number
in the file name corresponds to the sample’s DSID
since these
are all simulation. For the data samples, the number corresponds
to the run number in which the data was collected.
Now let’s look at the content of one of the simulated samples
using a TBrowser
:
You will see almost all of the same branches that are in your locally-produced ntuple as well as a large number of additional branches.
In addition to the electron (el
), muon (mu
), and jet (jet
)
object branches, you also see branches for tau leptons (tau
)
and photons (ph
). You also see additional met
branches as
well as branches holding information about trigger decisions.
Note that the ntuples contain tau and photon information even though they are not used in the analysis. This is generally considered bad practice because it adds size to the ntuples needlessly. Additionally, the inclusion of unneeded objects can impact the overlap removal procedure in a way that is not optimal for the analysis.
In this version of the ntuple, the
met
branches are vectors of floats, but this is not strictly necessary.
There are also several branches that end with NOSYS
, which
indicates that these represent nominal values without any
systematic variations considered. More details about storing
systematic variations will be presented in the systematic uncertainties section.
Furthermore, most physics object collections contain select
and effSF
branches. The former indicates whether each object
in the collection passes the selection criteria of a working
point and overlap removal for a particular systematic variation
(nominal in this case). Only objects that pass at least one
systematic variations are kept, those failing all available
variations are discarded. The latter is a scale factor that
needs to be applied on an object basis to correct for differences
between simulation and detector data.
Finally, the generatorWeight
branch includes weights that
need to be applied to each simulated event to account for
NLO contributions as well as scaling the simulation to the
expected yields in data.
The data samples do not contain any scale factor or weight branches.