Difference between revisions of "February 26, 2014 Calibration"

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(Minutes)
(Minutes)
Line 39: Line 39:
 
#** There are 120 channels in the microscope.
 
#** There are 120 channels in the microscope.
 
#** There should be 5 parameters per channel for the timewalk correction.  The exact form of the correction is to be determined.
 
#** There should be 5 parameters per channel for the timewalk correction.  The exact form of the correction is to be determined.
#**
+
#** The high and low energy bounds for each channel in terms of the fraction of the endpoint energy should be stored.
 +
#** The endpoint energy as determined in conjunction with the pair spectrometer should be stored.
 +
#** The fixed array will need similar constants, it has 220 channels (?)
 +
#* The active collimator is not needed for offline reconstruction
 +
#* Pair spectrometer (PS):
 +
#** The fine-segmented PS is purely hit-based, it checks for hits in coincidence gated with the coarse-grained PS.
 +
#** The coarse-grained PS has 8+8 channels, each with an fADC250 channel and TDC channel, with the respective constants needed for each of them.
 +
#** The gating threshold may also be needed for reconstruction.
 +
#* Total absorption counter
 +
#** 8 phototubes viewing a large block, each tube needs t0, gain factor, timewalk correction
 +
#* Polarimetry will be discussed in the future.
 +
#*

Revision as of 18:07, 26 February 2014

Meeting Time and Place

Wednesday January 15, 2013 at 11:00 AM. At Jefferson Lab, the meeting will be held in F326

Connections

To connect from the outside, please use ESNET

  1. ) ESNET: 8542553
  2. )To connect by telephone, dial:
  • You can look up toll-free number at http://www.readytalk.com/intl
  • US and Canada: (866)740-1260 (toll free)
  • International: (303)248-0285 (toll call)
  • enter access code followed by the # sign: 3421244#

Agenda

  1. Announcements
  2. Status Update
  3. Tracking
  4. Calorimetry
  5. Other systems
    • Photon Beam
  6. Simulations and Calibrations

Minutes

Attending: Sean, Amiran (NU); Curtis (CMU); Simon, Beni, Mike, Eugene, Lubomir, Mark I. (JLab); Zisis (Regina); Richard (UConn); Justin (MIT)

  1. Status Update
    • Not much new since the Collaboration Meeting last week.
    • Sean proposed to have a few dedicated meetings for the purpose of integrating the constants into the reconstruction and simulation codes after the upcoming data challenge.
  2. Tracking
    • Naomi reported (in absentia) that she is generating the Garfield tables needed for the CDC time-to-distance relations.
  3. Other systems
    • Richard described the current ideas of what constants will be needed for the photon beamline detectors. There is a wiki page on this subject that he will provide a link to.
    • Discussion started with the tagger microscope
      • Each fiber is associated with a TDC and fADC250 channel. The TDC will need a time offset, and the fADC will need a gain factor and time offset.
      • The ADC pulse shape will be used to match fADC and TDC hits, and the ADC pulse height will be used to determine timewalk corrections for the TDC hits.
      • There are 120 channels in the microscope.
      • There should be 5 parameters per channel for the timewalk correction. The exact form of the correction is to be determined.
      • The high and low energy bounds for each channel in terms of the fraction of the endpoint energy should be stored.
      • The endpoint energy as determined in conjunction with the pair spectrometer should be stored.
      • The fixed array will need similar constants, it has 220 channels (?)
    • The active collimator is not needed for offline reconstruction
    • Pair spectrometer (PS):
      • The fine-segmented PS is purely hit-based, it checks for hits in coincidence gated with the coarse-grained PS.
      • The coarse-grained PS has 8+8 channels, each with an fADC250 channel and TDC channel, with the respective constants needed for each of them.
      • The gating threshold may also be needed for reconstruction.
    • Total absorption counter
      • 8 phototubes viewing a large block, each tube needs t0, gain factor, timewalk correction
    • Polarimetry will be discussed in the future.