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Supernova Hack Days Summary Tom Junk LArSoft Coordination Meeting - PowerPoint PPT Presentation

Supernova Hack Days Summary Tom Junk LArSoft Coordination Meeting August 2, 2016 Participants Kate Scholberg (organizer) Erin Conley Jason Stock Diana Navas Chiara Lastoria July 25 July 27, 2016 Justin Vasel Fish Tank AJ Roeth Evan


  1. Supernova Hack Days Summary Tom Junk LArSoft Coordination Meeting August 2, 2016

  2. Participants Kate Scholberg (organizer) Erin Conley Jason Stock Diana Navas Chiara Lastoria July 25 – July 27, 2016 Justin Vasel Fish Tank AJ Roeth Evan Stewart Amanda Weinstein Steve Gardiner Alec Habig Chris Backhouse Denver Whittington Gleb Sinev Alex Himmel (remote) Tingjun Yang Tom Junk 2 8/2/16 Tom Junk | Supernova Hack Days

  3. Goals • Find energy and angle resolutions for low-energy electrons and photons generated with the particle gun and existing reco tools (last done by Z. Li) • Incorporate MARLEY into LArSoft (text files, and more elaborate software interface) • Run existing SNB simulation (Gleb, AJ, GENIE) and find energy resolution from - summed ADC charge - hit charge - space points with charge from PMA reco • Evaluate the angular resolution from reconstructed tracks • Make response matrices to incorporate into SNOwGLoBES • Study elastic ve+e -> ve+e scattering 3 8/2/16 Tom Junk | Supernova Hack Days

  4. Goals • Port NOvA's GENIE-based SN vector generation module to LArSoft's GENIE instance. One bit of value-add here is to get a time-ordered sequence of neutrino events sampled from the "light-curve". GENIE doesn't know about time-varying fluxes. • Make a library of photon-detector waveforms with SNB events with and without 39 Ar events, to help the DAQ group study triggering, Zero-Suppression, and compression algorithms • Run MARLEY in LArSoft and look for nucleon emission. Look at reconstructed energy resolution for events with and without nucleon emission • Identify low-energy photons and include them in the energy reco • Evaluate the impact of spatial dependence of impurity concentrations affecting the lifetime and thus energy resolution 4 8/2/16 Tom Junk | Supernova Hack Days

  5. Process • Preparation is important in order to maximize use of time – task proposals and homework worked great. • Tingjun and Tom helped solve technical issues and provide advice. • A spectrum of how aware participants were of the existing reco tools. More familiarity with simulation tools. • Participants were able to run standard MCC 6.0 workflows on SNB events and make event displays. Some issue with pedestals and zero suppression identified that affect the event display. • We tried out Gallery! And a request to try out igprof. Needed installation (both are available on scisoft.fnal.gov, but we should maintain installs on /grid/fermiapp) 5 8/2/16 Tom Junk | Supernova Hack Days

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  7. J. Stock 7 8/2/16 Tom Junk | Supernova Hack Days

  8. Steve Gardiner 8 8/2/16 Tom Junk | Supernova Hack Days

  9. Alec Habig, Justin Vasel 9 8/2/16 Tom Junk | Supernova Hack Days

  10. CLS="Cute" (or just "Crummy") Little Stub CLS Reco using PMA – Chiara Lastoria (actually particle gun: 10 MeV electron) MC Truth: points PMA Track: line 10 8/2/16 Tom Junk | Supernova Hack Days

  11. Reco algs may need optimization for SNB CLS Reco using PMA – Chiara Lastoria events. Different strategies for energy and angle may be optimal. ADC sum vs. tracking for example. 11 8/2/16 Tom Junk | Supernova Hack Days

  12. CLS Reco using PMA – Chiara Lastoria 12 8/2/16 Tom Junk | Supernova Hack Days

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