Simulation Data in High Energy Physics
Published November 1, 2022 | Version v1
Dataset Open

MicroBooNE BNB Inclusive Overlay Sample (With Wire Info)

Creators

  • 1. Tufts University
  • 2. Illinois Institute of Technology
  • 3. University of Cambridge
  • 4. The University of Manchester
  • 5. University of Texas, Arlington
  • 6. Tel Aviv University
  • 7. Fermi National Accelerator Laboratory
  • 8. University of Oxford
  • 9. Massachusetts Institute of Technology and Tel Aviv University
  • 10. Harvard University
  • 11. Syracuse University
  • 12. Brookhaven National Laboratory
  • 13. Lancaster University
  • 14. University of Michigan
  • 15. Kansas State University
  • 16. Columbia University
  • 17. University of California, Santa Barbara
  • 18. Colorado State University
  • 19. SLAC National Accelerator Laboratory
  • 20. Massachusetts Institute of Technology
  • 21. Wright Laboratory, Department of Physics, Yale University
  • 22. Centro de Investigaciones Energeticas, Medioambientales y Tecnologicas
  • 23. Universitat Bern
  • 24. University of Pittsburgh
  • 25. University Southern Maine
  • 26. Wright Laboratory, Department of Physics, Yale University and Fermi National Accelerator Laboratory
  • 27. Los Alamos National Laboratory
  • 28. University of Minnesota
  • 29. Universidad de Grenada
  • 30. University of Tennessee and Los Alamos National Laboratory
  • 31. Center for Neutrino Physics, Virginia Tech
  • 32. University of Cincinnati
  • 33. Rutgers University
  • 34. University of Edinburgh
  • 35. University of Warwick
  • 36. South Dakota School of Mines and Technology
  • 37. University of Chicago
  • 38. New Mexico State University
  • 39. University of Tennessee
  • 40. Louisiana State University

Description

MicroBooNE samples are provided for collaborative development in two different formats: HDF5, targeting the broadest audience, and artroot, targeting users that are familiar with the software infrastructure of Fermilab neutrino experiments and more in general of HEP experiments. The HDF5 files are stored on Zenodo, together with a list of artroot files accessible with xrootd.

This sample includes simulated interactions of neutrinos from the Booster Neutrino Beam (BNB), overlaid on top of cosmic ray data. The sample is inclusive, i.e. it includes all types of neutrinos and interactions, with relative abundance matching our nominal flux and cross section models. Interactions are simulated in in the whole cryostat volume.

The HDF5 files in this sample include the information at the wire waveform level (after deconvolution and finding of regions of interest). As this information significantly increases the file size, this sample contains about 17% of the events of the corresponding sample without wire information.

More documentation, including detailed description of content, recipes, and example usage, at https://github.com/uboone/OpenSamples.

Suggested text for acknowledgment is the following:
We acknowledge the MicroBooNE Collaboration for making publicly available the data sets [data set DOIs] employed in this work. These data sets consist of simulated neutrino interactions from the Booster Neutrino Beamline overlaid on top of cosmic data collected with the MicroBooNE detector [2017 JINST 12 P02017].

In addition, we request that software products resulting from the usage of the datasets are also made publicly available.

Notes

This data set was prepared by the MicroBooNE collaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. MicroBooNE is supported by the following: the U.S. Department of Energy, Office of Science, Offices of High Energy Physics and Nuclear Physics; the U.S. National Science Foundation; the Swiss National Science Foundation; the Science and Technology Facilities Council (STFC), part of the United Kingdom Research and Innovation; the Royal Society (United Kingdom); and the UK Research and Innovation (UKRI) Future Leaders Fellowship. Additional support for the laser calibration system and cosmic ray tagger was provided by the Albert Einstein Center for Fundamental Physics, Bern, Switzerland. We also acknowledge the contributions of technical and scientific staff to the design, construction, and operation of the MicroBooNE detector as well as the contributions of past collaborators to the development of MicroBooNE analyses, without whom this work would not have been possible. For the purpose of open access, the authors have applied a Creative Commons Attribution (CC BY) public copyright license to this submission.

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