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Exploring CMS Data Analysis Tools for Particle Physics Experiments

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5 diapositives · 116 Views · Jan 07, 2020

Learn about types of data in CMS software components, analyze generated particles, energy depositions, and reconstruction algorithms. Follow steps to employ SimTracks, Digis, RecHits, DST Objects, and visualization tools. Discuss energy resolution, tracking algorithms, and dataset exploration.

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Exploring CMS Data Analysis Tools for Particle Physics Experiments
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  1. Types of Data • SimTracks: generated particles • SimHits: energy depositions in a detector volume • Digis: Single-channel pieces of the detector’s raw binary output • RecHits: Reconstructed energy and position for a single detector elements • DST Objects: Higher level things, like jets & tracks

  2. Software Components • Generator (such as PYTHIA) • Creates SimTracks • Stores in PAW ntuples in a standard format (HEPEVT) • Simulation (OSCAR) • Swims the tracks through the detector, leaving energy deposits (SimHits) • Fast simulation (FAMOS) • Uses parametrized resolutions to smear the SimTracks, and make higher level (DST) objects • Reconstruction (ORCA) • Simulates detector signals (Digis) from the SimHits • Reconstructs (RecHits) & higher level (DST) Objects • Can run on these objects to make ROOT trees • Visualization (IGUANA)

  3. Starting out with CMS software • First place to start is the ROOT file • Get account on Fermilab analysis machines • Pick your favorite dataset • Single-particle sets are fine for now. • Start with a “Digi” or “DST” dataset, not “SimHits” • Follow the instructions in Eric’s talk to run ExRootAnalysis • Make ROOT plots of everything that might interest you • Pick out the calorimetry clusters in some eta/phi radius around certain type of generated particle • See what kind of energy resolution you’re getting • Can you see brem effects in electrons? • How is energy shared between ECAL & HCAL? • How does it depend on eta? • How many generated tracks are there around this particle? • Do they come from pileup? Underlying event? • How many reconstructed tracks?

  4. Learning about reconstruction algorithms • Try to figure out which algorithms make your favorite reconstructed object • “grep”ping through the codebase is your easiest option • DON’T try to follow the logic of how ORCA actually calls that algorithm • Look through CMS notes for reconstruction algorithms • (don’t expect much documentation for the code) • See what parameters can be varied in the .orcarc • Put some “cout” statements in, scram build, and run ExRootAnalysis again • Run from a “Digi” dataset this time, to make sure everything gets rebuilt. The “DST” dataset will already have the objects, so they won’t get rebuilt.

  5. New Framework • Timescale is spring/summer 2006, for cosmics tests • More rigidly-structured than ORCA • Data is “pushed”, not “pulled” • Stored in ROOT format, so you can plot the data directly from ROOT