Proton Calorimetry/Meetings/2017/01/25: Difference between revisions

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** Drop in gain somewhere around 20kHz.
** Drop in gain somewhere around 20kHz.
* Finished analysing Caen ADC and waveform data from November 2016 runs:
* Finished analysing Caen ADC and waveform data from November 2016 runs:
** [http://www.hep.ucl.ac.uk/pbt/wikiData/presentations/2016/clatterbridge_nov2016_analysis.pdf]
** http://www.hep.ucl.ac.uk/pbt/wikiData/presentations/2016/clatterbridge_nov2016_analysis.pdf
** [http://www.hep.ucl.ac.uk/pbt/wikiData/presentations/2016/clatterbridge_nov2016_waveform_analysis.pdf]
** http://www.hep.ucl.ac.uk/pbt/wikiData/presentations/2016/clatterbridge_nov2016_waveform_analysis.pdf

Latest revision as of 14:56, 25 January 2017

Minutes for UCL Proton Calorimetry Meeting, 25th January 2017 (D17, Physics & Astronomy, UCL)

Present

Simon Jolly, Anastasia Basharina-Freshville, Andreas Christou, Adam Knoetze, Matthieu Hentz

AC:

  • Working on analysis of scope waveform data.
    • ROOT will now identify bad pulses!
    • ROOT TSpectrum will analyse waveforms for double peaks based on histogram distribution.
  • Will next try and fit to good waveforms to train pulse filtering and integration.
  • Anastasia suggests looking at low and high rate files with no absorber.
  • Will also complete Java code to import binary files directly into ROOT: need to include input arguments.

AK:

  • Looking at various output spectra from Caen detector emulator.
  • Trying to set spectrum of waveform magnitudes (Caen instructions plus trial and error...).
  • Taking average of "large" waveforms to produce mean waveform for emulator.
  • Detector emulator time resolution much coarser than scope data (~160MHz): need to extract subset of individual waveform data to produce approximation of our waveforms.
  • Next step is to put output of detector emulator into digitiser and try and recreate Clatterbridge results.
  • Will also replicate Anastasia's experiments with LED light pulser injected into scintillator+PMT.

MH:

ABF: