Proton Calorimetry/Meetings/2016/11/30: Difference between revisions

From PBTWiki
Jump to navigation Jump to search
No edit summary
No edit summary
Line 12: Line 12:


'''AK''':
'''AK''':
* Converted August 2016 scope data from binary: data on <code>/unix/pbt</code>.
* [http://www.hep.ucl.ac.uk/pbt/wikiData/presentations/2016/AKnoetze_30.11.2016.pdf Converted August 2016 scope data from binary: data on <code>/unix/pbt</code>.]
* Not sure if timebase conversion is working correctly: will try and train conversion code on November 2016 Clatterbridge data.
* Not sure if timebase conversion is working correctly: will try and train conversion code on November 2016 Clatterbridge data.
* Detector emulator producing waveforms with various time distributions: able to provide custom time distributions.
* Detector emulator producing waveforms with various time distributions: able to provide custom time distributions.

Revision as of 16:13, 11 January 2017

Minutes for UCL Proton Calorimetry Meeting, 30th November 2016 (D17, Physics & Astronomy, UCL)

Present

Simon Jolly, Laurent Kelleter, Adam Knoetze, Matthieu Hentz, Anastasia Basharina-Freshville

AC:

  • Looking through waveform files for bad waveforms.
  • No bad waveforms found searching by eye: ABF suggests using a higher rate dataset in order to increase the chances of finding bad waveforms.
  • Will look at filtering peaks using built-in ROOT functions and throw away waveforms with double pulses.
  • SJ will provide Matlab scripts for reading scope data: aim is to reconstruct energy spectra for scope data from 24th/25th November 2016 Clatterbridge run.

AK:

MH:

ABF:

  • Working through data from November 2016 Clatterbridge run.
  • Still see amplitude reduction at high rates, with the added Brucie Bonus of an amplitude increase around 200kHz...

LK: