Difference between revisions of "CREXAuxiliaryMeasurements-Aug2020"

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#* S0 trigger
 
#* S0 trigger
 
#* production raster and beam position
 
#* production raster and beam position
<!--- # <font color="blue">Optics Data</font>  
+
# <font color="blue">Optics Data</font>  
#* retake watercell,  
+
#* Sieve IN, dp=+1, 0, (maybe -1).  Raster/no raster thin C, raster H20
#* retake optimization data
+
#* See grid on [https://docs.google.com/spreadsheets/d/1SngpqgLLULtcuKD0t9k-A2Cpmxy1jb5bIYnnP8f8zPM/edit?usp=sharing optics data spreadsheet]
#* inelastic spectrum data --->
 
  
 
== Backgrounds ==
 
== Backgrounds ==

Revision as of 12:26, 12 September 2020


CREX Main << August 2020 CREX Run Plan


WORK IN PROGRESS

  1. Please don't worry if there is a needless test on here, or an important one missing, or bad prioritization.
  2. Lets fix it

Optics and Q2

  1. Energy Measurement (Doug) (non-invasive)
    • I think this is complete. I need to check with Doug.
  2. Q2 measurement
    • Repeat of Q2 measurement, with improved pedestal noise control.
    • Detector counting mode.
    • S0 trigger
    • production raster and beam position
  3. Optics Data

Backgrounds

  1. Blinded Quartz
    • Longish access to setup and back out, but short data taking period (production conditions).
    • Reconfigure AT detectors to use blinding cap, attach to US PMTs.
    • This will be done during the long beam studies break on Monday
    • Integrating measurement for asymmetry measurement
    • Counting mode measurement for rate?
    • Can we make a plan for yield measurement? Maybe use absolute table top gain measurements?
  2. Rescattering measurement (~1 shift)
    • Needs a detailed run plan
    • measure to low dp~15%. Integrating mode? May require bootstrap on detector gain?
    • should scale all spectrometer magnets (including septum)
    • Once the elastic peak is out of the focal plane, it may be possible turn on the S3 and S0 scintillator. This should be done when possible, and the T1/T2/T3 trigger rate recorded for each run.
  3. Pole tip re-scattering
    • Requires investigation or planning - do we have an idea here?
    • Q2 or septum mis-tune, to increase interception on pole tip and improve poletip rescattering estimate

Detectors

  1. Linearity Studies (PITA + current scans)
    • These are ongoing - should continue regularly. ~ 1 hour every 3 days.
    • Current scans for detector and BCM pedestals
  2. Linearity LED tests
    • This will be studied post run, during SAD

Other

  1. Sign check
    • perform at next Moller polarimeter measurement
    • run Moller, Compton, and parity DAQ for quick PITA scan
  2. Target/Raster study


Moller polarimetry

  1. One more measurement

Compton polarimetry

  1. Flip DOCP???
  2. No-target runs
  3. Laser polarization optimization
  4. Laser polarization flip
  5. linearity studies