EPD Meetings

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EPD Meetings
Thursdays 08:30 (BNL time)

Meeting Zoom

 https://lehigh.zoom.us/j/93334661391?pwd=b1hpY3lPK3hPM0tCM2d0YUZOYk96UT09




Meeting 27 October 2021 (830 am EST)

  1. Run 22 EPD install
  2. Operations Run 22
  3. Calibration progress
  4. 19.6 GeV production issues?
  5. AOB
     
Meeting 12 August 2021 (830 am EST)
  1. EPD Small Systems - Jordan Cory - drupal.star.bnl.gov/STAR/system/files/Cory%20EPD%20Meeting%208-12.pdf
  2. Calibrations
  3. AOB


Meeting 1 July 2021 (830 am EST)

  1. EPD Removal Plan
  2. Calibrations
  3. AOB

Meeting 3 June 2021 (830 am EST)

  1. EPD Current Status
  2. Calibrations
  3. AOB


Meeting 13 May 2021 (830 am EST)

  1. EPD EQ3 Issues and OO Running - drupal.star.bnl.gov/STAR/system/files/RReedEPD05132021.pdf
  2. EPD EP Resolution
  3. Calibrations
  4. AOB

Meeting 6 May 2021 (830 am EST)
  1. dN/dphi - Xiaoyu - drupal.star.bnl.gov/STAR/system/files/EPD05062021.pdf
  2. Run 21 Calibrations
  3. Run 21 OO Running
  4. AOB


Meeting 11 March 2021 (830 am EST)

  1. Beamline Offset - Xiaoyu
  2. Run 21 -
  3. AOB



Meeting 19 June 2017

Rosi: drupal.star.bnl.gov/STAR/system/files/RReedEPD06192017.pdf
More complete analysis, including PDFs of all 93 channels and their associated ADC, TDC and TAC values can be found at: drupal.star.bnl.gov/STAR/blog/rjreed/auau-54-gev-triggers-and-eval-part-1
For those who may be interested in vertexing, multiplicity in the 54 GeV data, look at (not to be discussed): drupal.star.bnl.gov/STAR/blog/rjreed/auau-53-gev-evaluating-performance

Mike: In Au+Au collisions at 54 GeV (much higher than the multiplicities that drove the design of the EPD), we expect very significant multi-hit events on the tiles.  In fact, this analysis based on central Au+Au collisions at 62.4 GeV published by PHOBOS, indicated that the average hit multiplicity on a tile would be greater than 1.

And indeed, this is what we see, as shown on the following page:
drupal.star.bnl.gov/STAR/blog/lisa/multi-mip-events-2017-epd-auau-54-gev

Most particles are not coming from single-hit events.  So, we will need to be careful not to show "real quick dN/deta distributions," as they will be way off.

Justin:
Fiber polishing and bundle creation at Lehigh
drupal.star.bnl.gov/STAR/system/files/Fibers%2C%20EPD%20Meeting%206-19-17.pdf
drupal.star.bnl.gov/STAR/system/files/SS%25231_Fibers%281%29.pdf

Sam:
Simulation update
drupal.star.bnl.gov/STAR/system/files/sim_EPD_update06192017.pdf


Meeting 5 June 2017
1) Mike: TDCvsTAC
It turns out that all QT channels have a TDC in addition to the ADC they put out.  Supposedly it is a 5-bit TDC, but Hank reports that he's only seen 4 bits fire (returned value 0..15).  I have verified this in the EPD QTB boards, and find that the TDC is linearly proportional to the TAC, in the one QTB board that has a TAC.  You may find the picture here:
drupal.star.bnl.gov/STAR/system/files/TDCvsTAC.png
This could be useful in data analysis, for ALL channels (even the QT32Bs that will not have TAC, which is 75% of the EPD channels in 2018+).  I expect (though it has not been tested) that we can require TDC not equal zero, and be looking at in-time hits..
The TDC information is now included in the StEpdTile data object.

The following plots are ADC distributions, where the blue curves correspond to TDC!=0 and the red curves are for TDC=0.
drupal.star.bnl.gov/STAR/system/files/ValidTDCstudy.pdf
The TDC would seem to be an excellent way to discriminate noise/out-of-time signals from real particles.  Much more convenient than an ADC threshold.....  Except for a couple of bins, where the behaviour is precisely opposite to that expected.  This needs to be investigated.

More detail: drupal.star.bnl.gov/STAR/system/files/TDCstudy.pdf

2) Polishing at Lehigh:
drupal.star.bnl.gov/STAR/system/files/FiberPolishing06052017.pdf
drupal.star.bnl.gov/STAR/system/files/FiberPolishing06052017_pics.pdf

Meeting on 5/22/2017

1) Prashanth: Short update/summary of the situation with the QTs and new FEEs
www.star.bnl.gov/protected/bulkcorr/prashanth/EPD/weeklymeetings/PrashanthS_05222017.pdf

www.star.bnl.gov/protected/bulkcorr/prashanth/EPD/weeklymeetings/PrashanthS_05222017.pdf


Meeting on 5/16/2017 - at BNL during STAR Collaboration Meeting
Tuesday evening at 6:30 with pizza
Current run
Construction Software Ahead
  • all - plans for remainder of 2017 run
  • toward a "standard set of procedures" for operations 2018+
  • AOB

Meeting on 5/08/2017

1) Rosi - BBC-EPD correlations: drupal.star.bnl.gov/STAR/system/files/RReedEPDBBCCorr05092017.pdf
BBC - EPD timing studies: drupal.star.bnl.gov/STAR/blog/rjreed/epd-timing-correletion-slew-correction-vs-bbc-ii
Trigger, etc.

2) Justin - Fiber polishing and testing at Lehigh:
On the hardware page under "Useful EPD Documents":   drupal.star.bnl.gov/STAR/system/files/Justin%20Polishing%20Testing.pdf
Also at: http://www.star.bnl.gov/protected/bulkcorr/prashanth/EPD/Polishing_Testing_Justin_05082017.pdf


Meeting on 5/01/2017


1) Rosi - EPD-BBC timing studies & QT32C spikes - drupal.star.bnl.gov/STAR/blog/rjreed/epd-timing-correletion-slew-correction-vs-bbc

2) Prashanth - status at STAR
Also, discriminator study: drupal.star.bnl.gov/STAR/subsys/epd/operations-2017/discriminator-threshold-scan

3) Rosi - status of trigger coordination, including trigger bit test, etc.

4) Gerard - status/plans for FEE upgrade drupal.star.bnl.gov/STAR/system/files/gain_change_update.pdf

5) Mike - status/plans of EPD construction at OSU

6) Mike - ADC spectra with TAC cut - drupal.star.bnl.gov/STAR/system/files/ADCfitsTACcut_Lisa28apr2017.pdf

7) All - availability for in-person EPD session at STAR Collaboration Meeting

8) All - Plans for the coming week




Meeting on 4/24/2017

1) Rosi's blog:
drupal.star.bnl.gov/STAR/blog/rjreed/epd-analysis-32b-vs-32c-timing-correlations-etc

One important point:  best START for QT32Bs is -8 and best START for QT32Cs is -20

2) Joey BBC-EPD
www.dropbox.com/s/rbgzbbuhqfev1kr/BBCEPDCorr.pdf

3) Mike timing
www.dropbox.com/s/bn5wpxxj8gmm2qv/Timing.pdf


EPD To-Dos:
1) Confirm 32C settings - Change Tier 1 file!
2) Threshold Scan (32B first, then 32C once the above is accomplished)
3) DSM Bit checking
4) Software in CVS?


Meeting on 4/17/2017

1) Prashanth (software)
Mike's StEpd analysis software: 
/star/u/lisa/StEpd/

Database related
https://drupal.star.bnl.gov/STAR/blog/sprastar/epd-offline-db-table
https://online.star.bnl.gov/dbExplorer/


Meeting on 4/10/2017

1) Status of QT32Cs - Prashanth, Rosi, Gerard, Hank(?)

2) Bias scan - Mike
drupal.star.bnl.gov/STAR/subsys/epd/operations-2017/bias-scan


Meeting on 4/03/2017

0) Status - Prashanth, all

1) Prepost 32c vs 32b

2) Gate scan + conclusions
drupal.star.bnl.gov/STAR/system/files/GateScan_1.pdf
Summary:
  • QT32B likes START=-8  (as we concluded before)
  • QT32C likes START=-20
  • we see the "left edge" of the drop-off reasonably well
  • Gate scan concluded
3) Update on mounting structure - Robert

4) Bias Scan - Rosi has produced files for analysis; Mike has not yet analyzed them.

5) Gerard, all: interpretation of QT32C messages

6) Dark current:

7) Rosi - IV scan histograms: drupal.star.bnl.gov/STAR/system/files/IvscanHistos_03_26_2017.pdf

7.5) Sam - First steps with GEANT4 EPD: drupal.star.bnl.gov/STAR/system/files/EPD_geantSTARSIM_0.pdf

8) (If time) - Rosi: First steps with UrQMD: drupal.star.bnl.gov/STAR/system/files/RReedEPD03272017.pdf


8.5) Rosi: Starting to look at BES data (7.7 GeV): drupal.star.bnl.gov/STAR/system/files/RReedEPD04032017.pdf

9) Tasks for the coming week.
  • From last week: 1,2 are done; 3 is canceled; 4 is done but not analyzed.  5....?
  • New tasks

Meeting on 3/27/2017

1) Prashanth, all:
  • Current problems - CAMAC PS?
  • Plans for access
  • do not swap QT32C inputs with QT32B for now (see "steps for this week" below)

2) Mike - Gate scan study
3) All: Next steps for this week
  1. get trigger guys to put us in PrePost=0
  2. continue gate scan to "more negative" values to find QT32C plateau and final gate delay value
  3. swap inputs of QT32C with a QT32B to check gain (why this is not already known from the lab...??)
  4. Bias scan
    • step size, range
    • what is figure of merit? "MIP position matching"?  Separation from dark current?
    • operationally - take-a-run, burn-a-run while switching, take-a-run...?
  5. TAC ajustment - will need Jack's help (Gerard will be at BNL?)

4) Dark current:

5) Rosi - IV scan histograms: drupal.star.bnl.gov/STAR/system/files/IvscanHistos_03_26_2017.pdf

6) Joey - BBC-EPD correlations - drupal.star.bnl.gov/STAR/system/files/EPD%20Presentation.pdf

7) (If time) - Rosi: First steps with UrQMD: drupal.star.bnl.gov/STAR/system/files/RReedEPD03272017.pdf




Meeting on 3/20/2017
1) Mike: PrePost study of runs 1806643, 18076064 and 18076065:
drupal.star.bnl.gov/STAR/system/files/Study18066043and18076064and18076065all.pdf
(This study under the Operations 2017 child page)

2) Mike: Draft (v1) of trigger documents shared with trigger group and to be discussed 21march2017:
drupal.star.bnl.gov/STAR/system/files/EPD%20Trigger%20Requirements%20v1.pdf

3) Mike: First Gate Scan study.  This will need to be revised, as discussed on first page of this document.
drupal.star.bnl.gov/STAR/system/files/GateScan_PrePostIndex2.pdf
(This study under the Operations 2017 child page)

Meeting on 3/13/2017
1) Mike: TAC-selected spectra from run 18067001: drupal.star.bnl.gov/STAR/system/files/Run18067001_spectra.pdf
Also, drupal.star.bnl.gov/STAR/system/files/FitValidTACadcSpectrum.pdf


Meeting on 3/6/2017
1) Mike: Spectra Fits from vbias 56.5V data: drupal.star.bnl.gov/STAR/system/files/MLisaEPDFits03062017.pdf

2) Rosi: Vbias comparison: drupal.star.bnl.gov/STAR/system/files/h_CompareVolt03052017_Vbias56_5_v3.pdf
How shall we set these values?  (Above needs to be repeated with the better vped values and with Jack's new Tier1 file.)


Meeting on 2/27/2017
1) Rosi - Tested the detector by increasing the Vbias in each channel by 5 V.  The dark current increased, one can see it at:
drupal.star.bnl.gov/STAR/system/files/h_DarkCurrentHistogram_Nhours149.pdf
The current increase is at the end.
Plot of the pedestal per channel:
https://drupal.star.bnl.gov/STAR/system/files/h_Ped18052002_v2.pdf
Only one channel is "fat" and it should be determined whether it is FEE, QT, or Receiver
Dark Current as of this morning:
drupal.star.bnl.gov/STAR/system/files/h_DarkCurrent_Nhours288.pdf
Gerard asked what happens if we decrease ymax to 0.3nA, see:
drupal.star.bnl.gov/STAR/system/files/h_DarkCurrent_Nhours288_ymax03.pdf
Lehigh schedule for WSL fibers:
drupal.star.bnl.gov/STAR/system/files/epd_schedule_Lehigh_WSL.pdf

Also note, Prashanth has added it to the online monitoring!

2) Prashanth - Timing in, inclusion to StRoot

3) Sam - Adding EPD to the STAR GEANT:
drupal.star.bnl.gov/STAR/system/files/Epd_Geant.pdf

Meeting on 2/20/2017
1) Rosi -
VPed Setting: Code is at
/gpfs01/star/subsysg/EPD/VpedDet/
Summary: drupal.star.bnl.gov/STAR/system/files/RReed_EPD_02192017_Vped.pdf
1 set of fits: drupal.star.bnl.gov/STAR/system/files/h_Vped.pdf

Vbias: Code is at
/gpfs01/star/subsysg/EPD/IVScan
Summary: drupal.star.bnl.gov/STAR/system/files/RReed_EPD_IVscan_02192017.pdf

Dark Current: Code is at
/gpfs01/star/subsysg/EPD/DarkCurrentMonitor
Summary: drupal.star.bnl.gov/STAR/system/files/RReed_EPD_IVscan_02192017.pdf
Scan at of 10:30 am: drupal.star.bnl.gov/STAR/system/files/h_DarkCurrentHistogram_EPD02202017.pdf
Note: I did an IV scan, which we can see the evidence of.  Also, I am unsure why one of the boards is not showing any movement.  I will check on this during the week.

Open questions: When can we be timed in? Shift crew instructions? Monitoring at: https://online.star.bnl.gov/epd/ ?  MuDst?

2) Prashanth -
online monitoring page here: https://online.star.bnl.gov/epd/

Notes: Prashanth is discussing with Akio the best way to incorporate our detector in the MuDsts.  The question is where does the mapping get picked up, which is currently being picked up in the trigger data.
Action items for Rosi:
*Test the detector by setting Vbias = Vbias + 5 V to see that the dark current has increased.
*Plot the pedestal distributions per channel.
*Touch base with Akio/Tonko about the functionality of the standby mode and whether it is needed for pedstal runs.
*Fix Vped for 3 channels not connected to an EPD tile
*Touch base with Prashanth to see what software tasks can be distributed so he can concentrate on incorporating the EPD into the MuDst
*Ask to have the IV Scan + Pedestals taken via the shift crew (pending the answer from Akio/Tonko).
We also discussed the need for documentation, at the moment things are a bit chaotic.  This will improve our ability to distribute tasks.

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