Supernova Hack Days Summary Tom Junk LArSoft Coordination Meeting - - PowerPoint PPT Presentation
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
Participants
Kate Scholberg (organizer) Erin Conley Jason Stock Diana Navas Chiara Lastoria Justin Vasel AJ Roeth Evan Stewart Amanda Weinstein Steve Gardiner Alec Habig Chris Backhouse Denver Whittington Gleb Sinev Alex Himmel (remote) Tingjun Yang Tom Junk
8/2/16 Tom Junk | Supernova Hack Days 2
July 25 – July 27, 2016 Fish Tank
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
8/2/16 Tom Junk | Supernova Hack Days 3
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 39Ar 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
8/2/16 Tom Junk | Supernova Hack Days 4
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)
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- J. Stock
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Steve Gardiner
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Alec Habig, Justin Vasel
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CLS Reco using PMA – Chiara Lastoria CLS="Cute" (or just "Crummy") Little Stub (actually particle gun: 10 MeV electron) MC Truth: points PMA Track: line
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CLS Reco using PMA – Chiara Lastoria
Reco algs may need optimization for SNB
- events. Different strategies for energy and
angle may be optimal. ADC sum vs. tracking for example.
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CLS Reco using PMA – Chiara Lastoria
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