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November 3

Phone bridge number 617 452-2163 , Time 5 pm to 6+pm pm, up to 10 connections
Agenda

  1. PPV , Rosi, solution to CMB problem - great job!
  2. TPC calib: Gene, Joe
    • SC &GL
    • tuning of TPX slow simu , needed for embedding
    • evaluation of chi2/track for M-C & data (again embedding)
  3. closing Endcap geometry - Ilya
  4. status of approval of embedding request - Bernd
  5. status of pythia-filtering - Bernd
  6. Generation of M-C events w/ 2009 geometry (efficiency, embedding)
    • shall we go privately with production
    • shall we pay for it to Amazon (how to find $5-10K ?)
  7. BTOW calibration: Joe + Matt
  8. Vernier scan: what W xSection have we measured in run 9, error discussion, Ross
  9. study of beackground, events reco : Justin & Scott
  10. progress on W->Jet+Jet+X channel
  11. AOB

October 27

Present: Justin, Joe, Ross, Will,Gene, Scott, Ilya,

  1. W-analysis plan shown to PWGC by Bernd
  2. Embedding plan - Jan, procedural steps:
    a) Present the same task list for completeness in tomorrows software meeting : Jan
    b) Present a brief update of this during the SPIN PWG meeting, in particular a statement about the question for embedding
  3. TPC calib (Gene, Joe): T0 loaded to Db, SC calibration started
  4. BTOW calib (Joe) : ~60 towers w/ mixed fibers will be masked as dead, not sure when all is uploaded to DB
  5. Ross , eta dependence of non-gaussianity
  6. Justin, Scott  Kinematics Transvers Mass

October 26 , special meeting to discuss Bernd's task list

Present:Gene, Bernd, Joe, Jan, Rosi,Justin, Ilya
Minutes

Bernd reported from the private meeting w/ Jerome. There is general good, common understanding of priorities.
From the list of 'red items' on Bernd's list 2 are problematic:

  • implementing deconvolution code would take months in real time , during meeting we have agreed to descope this item
  • commissioning of MC filter. Jerome plans to personally review the code, not sure when it may happen. Jan made suggestion to delegate this task.
  • ETOW geom is ~done for Jerome. However Ilya confirmed it is 'not right' for IUCF. the new SF=4.7% changes by 6% in the wrong direction if XXX? is changed in geometry. A week+ is needed to resolve it.

Rosi confirmed the T0 fix did not helped in restoring CMB tracks in PPV. She will try to investigate it further, but asked for new ideas. So far nothing is wrong. It was not confirmed CMB tracks are missing also for M-C events. This item has no ETA.

Joe & Matt realized the mip-less towers w/ good slope have either wide pedestal, or low gain, or unstable HV, or all of the above (the spectra and detailed rapport will be posted). All such towers will have offline gains determined from the slopes (are restored). Now we will have only ~100 dead towers in BTOW. List of those will be posted on emc2-hn , so there is a record, perhaps some can be repaired before the run. No evidence of the elusive towers with mixed fibers. This item is declared to be resolved.

Gene reported T0 fix is in DB. Today Joe can start working on SC & GL calibration. ETA 1 week, perhaps longer. The 'stop condition' is achieved residuals in sDCA below 0.3mm.

Revelation: once SC & GL are in DB, Jan need to run pilot production so Rosi can re-examine beam line constrain and upload those to DB. Total ETA ~3 days.

Ross prepared his (& my) first guess of systematic errors contributing to the Xsection, see last item below.
For now the outstanding item (20%) is due to the gauss shape? used in the V-scan fit. We need more details (plots, comparisons) to discuss it.

Embedding - using it would address several uncertainties at once:

  1. loss of true Ws due to pileup tracks or EMC hits in either of the veto-cones
  2. in particular beam-background tracks affect veto in the Endcap
  3. amount of contamination to reco Ws due to accidental pileup track pointing to trigger pi0 cluster
  4. contamination due to non-collision trigger messing up lumi calculation
  5. loss of track efficiency due to removed clusters tagged on-line as deconvoluted, here beam background also plays the role

Significant time was spent arguing w/o concrete arguments:

  • one could approximate X by Y, but not sure how accurate will it be done, vs.
  • I want either embedding or deconvolution, because I do not trust anything else
    This is representative to expected discussion on a broader forum and affected my suggestion how to proceed.

Material used during discussion

  1. Bernd (obsolete now) analysis task list is at:http://drupal.star.bnl.gov/STAR/system/files/W-analysis-tasks.pdf
  2. Carl's arguments for embedding:http://www.star.bnl.gov/HyperNews-star/protected/get/starspin/3953/2/1/1.html
  3. Pibero's embedding request for pp200 data , run 9http://www.star.bnl.gov/protected/spin/pibero/dijets/2009.10.23/embedding.html
  4. 'OLD' embedding requests in the queue: http://drupal.star.bnl.gov/STAR/comp/embedding/operations/old-requests
  5. Procedure of requesting embedding, as described by Renee (the Embedding team leader)http://www.star.bnl.gov/HyperNews-star/get/embedding/658/1/1.html
  6. access to ZB events for many run in pp500 is painful, often there is no separate event stream:http://www.star.bnl.gov/HyperNews-star/protected/get/rts/298/1/1.html
  7. Ross: sources of systematic error for W X-section

October 20

Present: Bernd, Jan, Ross, Will, Scott, Justin, Ilya
Minutes

  1. Vernier scan analysis, trying to reconcile fast and vernier cross sections through z dependence - Ross
    Understanding of discrepancy between ZDC vs. BHT3 may require a trip to BNL, but for next week we should expect 1st estimation of W Xsection from run 9 data with detailed table of all systematic errors.
  2. Update on Transverse Mass Reconstruction - Justin  blog
    After code fix rec transverse mass for M-C (fig 5) and data (fig 7) look more alike
    Fig 6 shows prospects of reco longitudinal momentum for Ws , today for M-C, will be tried w/ run 9 data soon
  3. AL for W-> di-jet, P.Nadolski predictions for LP^2 FOM=80/pb : PDF page 30
    UA2: L=0.7/pb, sqrt(s)=630 GeV, p+pbar : see W yield on PDF page 17.
    Q: compare seen # of Ws for UA2 vs. expectation for STAR run 9.
  4. Bernd - Latex paper new deadline : Monday, October 26 for Jan, Scott,Ross, Bernd
  5. Jan - update on deploying STAR software on Amazon Compute Cloud (EC2) , first bill
  6. Postponed for next week
    • TPC - status of calibration
    • TPC - status of handling of deconvoluted hits by Sti
    • PPV - understanding of missing CMB tracks
    • BTOW absolute calibration: mip-less & slop-less towers
  7. Announcements
    • Ilya (IUCF) signed-on for W2009-mailing list

October 13

Present: Hal, Jan, Ross, Will, Scott, Justin, Dave.

Proposed 2010 Spring APS abstracts:
  1. Overview of the STAR W spin physics program in polarized proton-proton collisions at ps = 500GeV at RHICT - Bernd
  2. Absolute Cross Section for W+ and W− Boson Production at sqrt(s) = 500 GeV at STAR - Justin
  3. First measurement of the parity-violating spin asymmetry AL for W± boson at STAR - Jan
  4. Determining sampled luminosity in proton-proton collisions at sqrt(s) = 500 GeV at STAR using the vernier scan technique - Ross

DNP W talk by Joe: final version
Ws measured by STAR in 2009 run

Minutes

  1. vernier scan agrees with Angelika in fitting time dependent shape, still disagrees with Bill on estimate of BHT3 xSection (blog)-Ross
  1. Justin - new away side veto blog
    Algo identifying 3-jet events: 3 independent seeds in TPC, BTOW, ETOW, take highest PT track away in phi, delPhi<90 deg, away cone delR<0.5, 2x2ET/coneET<0.3. Rejected 9 events from run 9 & large 2x2ET.
  2. Jan - model of Jacobian peak w/ 3D Gauss smearing blog
  3. Scott - longitudinal smearing of initial-state parton momentum blog 
  4. Longitudinal initial state momentum reflect in reco p_Z for Ws blog, Justin

September 29

Present: Hal,Joe, Ross, Jan, Scott, Justin, Gene
Minutes

  1. TPC calibration - Gene: T0 did not fixed CMT problem, PPV need investigation
  2. BTOW absolute calibration - Matt
  3. figures to be released as 'STAR Preliminary' for DNP - Joe - link
  4. Vernier scan update - Ross
  5. h /h- ratio for QCD, Ws - Justin
  6. uploaded spin DB for pp500 short , longer- Jan
  7. AL for W+ - Jan
  8. W paper 1 - Bernd
  9. AOB
  10. Announcements
  11. updated run list w/ pol pattern pp500-runList-ver4.csv

September 22

Minutes

  1. PPV - status of evaluation of SL09b production, missing CMB tracks
    PPV blog:
  2. TPC calibration - Gene
    • when can we replay data for one fill?
  3. BTOW calibration
    • relative are done, or ? (smile) - Joe
    • absolute : E/P using slopes & ideal gains - Matt
  4. W analysis
    • Joe - updates? Close to final version to be shown on Thursday.
    • Justin -
  5. W paper 1 - Bernd
  6. CNI polarization of protons during 500 GeV run (Data files: ): Yellow Fill dependence: and Blue Fill dependence: - Bernd
  7. Background Estimation - link
  8. AOB
    • Ws from Phenix

      There are no images attached to this page.

      There are no images attached to this page.
  9. Announcements
    • Hal finished run QA for fills: 10383,10389,10399, 10402. We are done!

September 15, 2009

Minutes
Present: Hal,Jan,Will,Ross,Joe,Bernd,Justin,Scott, Gene

  1. TPC - Gene reported slewing correction for clusters is in DB. T0 should be in DB at the end of the week. Then we can ask for re-production of one fill to see if tracking efficiency improved at Z~0
  2. PPV - status of evaluation of SL09b production - no report
  3. Vernier scan - Ross
    • formula computing BBC xsection seems to be complete now. For a low lumi fill in pp500 the computed BBC xsection is 26mb - close to the value know for pp200
    • Q: what do we expect for BBC xsection at 500 GeV - answer is unknown
    • the linear formula can't be applied for regular fills when BBC is saturated, Hal suggested using more advanced approach counting bXings w/o rate, using zero of Poisson distribution. LINK SHOULD BE HERE
    • BHT3 x-section : results of fit with noisy patches removed Conclusion: background reduces but not vanishes. Comparison for other vernier scan will be made, estimation of error in determination of xSection due to non vanishing background will be made
  4. BTOW calibration
    • relative -Joe - link , is completed. Write-up was sent to emc2-hn for comments.
    • absolute -Matt, will be performed shortly using Joe's relative gains.

  5. Understanding QCD e+/e- ratio at ET [15,20] GeV - Scott.

    • Plan: use Pythia events and simplified W-algo to determine the ratio of high pT particles with positive/negative charge.
    • Manpower: not assigned.
  6. Status of W analysis:
    1. Joe detailed presentation of alternative W-algo, run 9 data & M-C - link. Results are consistent with Jan's analysis. 2 independent algos leading to similar output improve confidence in the result.
    2. Jan's ver 4.2 : bug fix, upgrade, answers to questions after last week spin PWG presentation , slides
    3. Justin : using ETOW in W-algo improves S/B in ET~20 GeV region, allows background estimation for di-jets escaping through not existing East endcap.
  7. Layout of paper 1: Draft: Files: Bernd
    Decisions:
    • Bernd will oversee the latex files, complete version will be posted in spin/protected/ area at THIS LOCATION
    • Assigned chapters: Intro+RHIC : Bernd; STAR : Scott; Lumi : Ross; Trigger : Jan
    • We hope to have them written by next week.
  8. Announcements
    • Hal finished run QA for fills: 10403, 10404, 10407, 10412.

September 8, 2009

Present: (I lost my notes, sorry)

  1. BTOW final 5% calibration
    • relative Joe- expected next Monday
    • absolute Matt- after Joe
  2. TPC
    • what is new in terms of calibration - Gene ,e.g. T0(amplitude) correction
  3. PPV - status of evaluation of SL09b production - Rosi
  4. Vernier scan - absolute BHT3 normalization - Ross
  5. W-background estimation based on run 9 pp500 data : Scott/Justin
  6. spin info : fill pattern, bXing offset - update (Jan)
  7. run QA (first week) Hal, left overs from later days Dave
  8. RHICBOS cross-section plots (Bernd)
    Summary: The ratio integrated over pT is:
    • W+ / W- = 5 / 1 at mid-rapidity,
    • total cross-section ratio is: W+ / W- = 3 / 1.
    • At forward-rapidity, the ratio is: 1.8 / 1
  9. Overview of previous W measurements Bernd
  10. task assignment (a.k.a Run 9 data publication strategy ) - please take responsibility
  11. Status of W analysis:
    1. Joe
    2. Jan's blog
  12. What do we show on Thursday to spin PWG, how many details?
    #AOB

September 3, 2009

Present: Scott, Justin, Joe, Willie, Jan, Ross, Bernd, Gene, Hal

Minutes

  1. result of analysis of SL09b production
    1. Jan (Drupal blog )
      1. presentation of W-algo ver 4.0 using BTOW & TPC, for 1M input events
      2. Run 9 results as of September 1 Slides
        1. histogram-based dump of selected events
        2. Larger collections of events: di-jets , W-candidates , Z-candidates
        3. Matt's 3 interactive events in skechup or just one view , at Scott's angle
        4. sequential histograms from pass through 1M events (LT=~8/pb)
      3. M-C simulation analysis histograms for Pythia W-events (LT=320/pb) , filtered QCD-events LT=6.3/pb, Z-events LT=4200/pb
      4. Suggestions: count # of track pointing to cluster; compare ET vs. PT for electron
    2. Joe adopted his algo developed on M-C to work with Run 9 data
      • removed BSMD, changed to tower-based center of gravity, relaxed cuts: PT>5 GeV/c, delEta & delPhi<0.5, isoFraction of 0.8
      • Uber-preliminary result for 1M input events results plots
  2. Run 9 data publication strategy has been discussed and in general agreed up. Use of BSMD for PRL paper 1 was discussed - it is worth trying.
  3. Questions/comments
    1. from former prominent STAR collaborator:
      • Could the Z-candidates be di-jets? cosmic rays? Do you try to do any charge sign discrimination on the electrons (i.e., opposite sign on the 2 sides for "Z-candidates")? Phi distribution does not appear indicative of cosmics.
      • Most importantly, is "Jacobian peak" absent when you look at 200 GeV data with the same algo and cuts?
      • Lots of questions, but this does look really promising, seems to give you NN W candidates NN Z candidates in the barrel region. It's a bit surprising that such a crude isolation cut, with no away-side ET upper threshold or SMD criterion, would suppress jet background so effectively. We always thought we would have to work much harder than this to unveil a signal above background.
    2. Jan: Lets plan to use BFC filter to get rid of not-BHT3 events from pp200 data. Process LT~10/pb. Needs: adopted filtering code, run selection, 1mm accuracy of TPC calibration (within month), supported production request
    3. Joe: estimate TPC tracking efficiency difference for e+ vs. e-
  4. Ross - vernier scan analysis
    1. lots of detail about how I do the fit - Ross is looking for explanation why his calculations are off by ~4 orders of magnitude. knows
    2. Comparison of Vernier scan from 2 pp500 runs - background visible in both
    3. Comments/suggestions:
      • post study with eliminated TP affected the most by the beam background - no link yet. Even removing the noisiest high tower patches still leaves considerable amounts of background. ADD LINK
      • post input data from Angelika Raw data from Angelika
      • exercise the code on mock data to verify it reconstructs width correctly
  5. Joe - BTOW relative gains, not yet
  6. new phone meeting time moved to : Tuesday 5-6 pm EDT
  7. low TPC tracking efficiency at eta~0. Gene: may by a better T0 suffice to correct it - lets wait for the outcome. How can we address this issue?

August 27, 2009

Present: Willie, Matt, Jan, Hal, Rosi, Justin
Minutes

  1. Evaluation of SL09b production
  2. TPC calibration, Gene: Could you describe realistic timeline for complete TPC calibration: PadrowT0, Twist, ShortedRing
    Next production should include all of the above
  3. ETOW gains - Scott/Justin
  4. BSMD relative gains - Willie, uploaded to DB with flavor Wbose
  5. Vernier scan - Ross, all 6 pp500 runs have been produced.
  6. Announcements
    • Jan: the following runs will be tagged as Xx because there is 0 or <100 events with found vertex :
      R10084013, R10088103, R10081024, R10095032, R10085022, R10088060, R10085103, R10087007, R10093049, R10085118
    • corrupted muDst: /star/data33/reco/production2009_500Gev_c/ReversedFullField/P09ib/2009/097/10097044/st_W_10097044_raw_6180001.MuDst.root

August 20, 2009

Present: Rosi,Hal,Jan,Justin,Gene,Ross

  1. Production status
    • pilot production has been QAed . No major problems were found and Lidia is most likely executing production now.
    • expect St-W muDst to be ready in few days.
    • identified problems to be fixed before next production
      • explain why PPV sees no tracks crossing TPC CM
      • why 7-bit bXing has no abort gap for the fill on page 19 top plot ?
  2. ETOW absolute calibration to compensate for incorrect TCD phase used during data taking. Two alternative methods are used:
    • Justin is comparing ratio of slopes for correct & incorrect TCD phase from regular minB events from pp200 data:http://drupal.star.bnl.gov/STAR/blog/stevens4/2009/aug/05/run-9-eemc-tcd-phase-and-effective-gains
      Fig 1.1 show example for 1 tower
      Link http://drupal.star.bnl.gov/STAR/system/files/ETOW_SlopeSet0vSet1234.pdf
      shows slopes (top) and the deduced gain correction (bottom) for all towers and all crates.
    • Scott is analyzing slopes from calibration pp500 data taken and various TCD phases and predicts similar gain correction for the TCD phase value used during W-data taking. The comparison is here

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      In particular pages 4-6 show error bars. Both methods lead to the same gain correction.
    • The plan is to compute weighted average gain correction and upload it to DB with a different flavor. So user will get non-sense gains for the default 'ofl' and needs to request those. (Very good plan, Jan)
  3. Status of Vernier scan was presented by Ross:http://drupal.star.bnl.gov/STAR/blog/rcorliss/2009/aug/20/absolute-cross-section-notes-5
    The rate of STAR events vs. time (fig 1) is described by the product of 2D gauss functions representing X,Y spread of ions in both (identical?) beams. We know from Angelika the relative displacement of both beams for every time period of Vernier scan. Ross fits 2 params: sigX, sigY - the width of gauss.
    Fig 3 ('counts vs. steps') shows anticipated result. The value of 'skfNN' is absolute cross section of STAR BHT3 trigger in units TBD and assuming no hot tower correction is needed.
    Ross add constant background to better describe the observed rate , yet still peaks are under-predicted.
    He will continue to try to model vernier scan better and is awaiting for muDst from 6 Vernier scan runs from ongoing production to be able to assess how stable is the value of skfNN.
  4. run QA : Hal will do QA of the first week of pp500 data within next 30 days, backward in time. (Thanks^2, Hal)

July 16

  1. Joe/Gene - spacecharge and gridleak - Having had Gene diagnose that there were issues with the gridleak in the current calibration I went back with his estimated numbers and re-ran it, but there may be problems with that now and it may take another iteration or two to find our way to the correct place to be.
  2. Hal - QA - Didn't call in, but he said at the analysis meeting that he would do more QA (the rest of it).
  3. Rosi/Jan - PPV - Rosi was working on the beam tilt part of it now and it sounds like she is getting good results and everything so it won't hold us up once we get the sc/gl ready.
  4. Willie - BSMD - Showed his progress (see the email he sent around)
  5. Ross - Vernier - See his drupal page
  6. Scott - ETOW gains - See his presentation. He started looking at the gains in each sector now with the data from the timing scans, but using "Scott's method" for calculating the gain (last slide). It looks like sectors 5 and 6 are actually different from 3 and 4 when you use "Scott's method". He thinks he will have a gain for each tower calculated by the end of next week though. So excellent progress there.

June, 25

Present: Gene, Scott, Joe, Jan, Willie, Ross,Rosi

  1. TPC, Gene:
    • TPC alignment used now is old, from run 8
    • Joe produced non-linear SC based on 10 runs , not yet in DB.
    • Units for SC are V/cm^2. Conversion to actual correction used to shift clusters is SC of 0.01 V/cm^2 --> 8.5mm of shift in the X-Y plane for track at eta=0.
    • Few days later Joe generated SC ver 2 based on ~60 runs and differences between SC ver 1 & ver 2 are of 2 mm at the highest ZDC rate of ~170 kHz
    • we need to check if after applying SC the residua are scattered around zero, using different runs
    • Gene will evaluate DCA to the vertex to see if we achieved 2mm accuracy of global tracking
    • Jan investigated chi2/dof for tracking (before SC were applied) and found its average is of 1.5. We discussed how to rescale TPC hit errors to get avr chi2/dof=1.<br> There are 3 critical parameters deciding how big are errors of clusters: *dip angle, * crossing angle, and *track momentum(?not sure?) <br> Few days later Jan check chi2/dof w/ Sc and it was much closer to 1 - perhaps rescaling of hit errors is not necessary.
  2. BSMD was never aligned with TPC for real data - brought by Scott. We could (should) use high pT electrons reco in TPC for alignment. L2W events will be ideal. Jan asked Matt about the change in BTOW geometry last year to add dead material at eta=0. Matt said this change did not affected BSMD geometry model, so we have in reco what we believed was true ca. 1998. It needs to be verified with actual 2009 data.
  3. ETOW gains: Scott got from Alice timing scan data and will analyze them. We discussed reliability of gains for towers with significantly wrong timing when gain correction factor is of 10 or more. It is important to look also at derivative of d_gain/d_timing and flag as bad towers with large correction or large derivative. Details TBD.
  4. beam line constrain: Rosi was finalizing 3D fitter based on Minuit. 3 days later: code is running but convergence is not great, few problems are identified, e.g. too many fit params. Rosi & Jan are working on this - top priority, needed for production to start.
  5. preparation for data production:
    • we want to run over 1.4M of L2W events vs. ~900 M of all events taken in run 9
    • Joe will give presentation motivating this production to PWGC
      #*Before we start production following must happen: <br>- confirmation non-linear SC does improve TPC accuracy<br> - mean chi2/dof should be ~1 <br> - beam line algo by Rosi, Jan must be developed, tested, vetted <br>- beam line algo must be executed over full pp 500 data set and beam line params loaded to Db<br>- problem w/ ADC=0 for ETOW for certain runs needs to be resolved , Ross reminded me it was discovered already in the past, if # of corrupted 'sth' was >40 the whole block was set to 0 - need half day of attention <br>- run list needs to be generated, including sub-list of daq files for the 5% sample-production - this is half day of my work
  6. run QA: ver 3 of run list incorporating peoples run QA prepared so far has been assembled: pp500 run list ver3c , 80% QAed, updated June 29

June 18, 2009

Present: Gene, Scott, Jan, Willie, Hal, Ross

  1. TPC, Gene:
    • non-linear SC(lumi) should provide TPC track accuracy of 2 mm at both ends of the track. We hope Joe will work on this next week, should take a week.
    • We could also use Gene's PCA method of finding a linear combination of scalers (each at first order).
    • since linear SC(lumi) was tuned to lumi equivalent to ZDC base rate of 70kHz, any pp500 run taken at the ZDC rate has current best TPC calibration. Jan: I'll use it for beam line constrain study, see below.

    • beam line constrain : plan A is Rosi & Jan succeed with 3D beam line fit to global tracks w/o intermediate vertex finding. Here are [[Media:Beamline-v3.pdf ]] as intended and not implemented. If this works Gene needs a ~day to produce beam line constrain for all 39 fills. Plane B is to use Minuit vertex finder which may require significant stats to overcome jitter due to pileup tracks. In such case we would need to provide manpower for ~week long job, Gene would only supervise it. Jan: lets go for plan A.

    • conclusion: once both items are resolved we can ask for production, perhaps 2 weeks from now.
  2. BTOW, ETOW gains - no progress.

  3. BSMD : Willie is working '''slopes for individual strips'''. He run over 10k VPD-minB events and got this [[Media:BSMD-strips-Picture 16.png]] and spectra [[Media:BSMD-strips-Picture 15.png ]]. The available 1.5M vpd-minB events should be enough to fit every strip. If not we will merge strips.

  4. BSMD geometry: Scott asked how well we know '''relative position of BSMD vs. TPC'''. It is followed up on emc2-hn . <p> Scott once did [[Media:Conversions-distace-Scott.pdf | simple calculation for photons that convert to e+/e- pairs]] in the SVT, attached. <br>The relevant equation is on the bottom left. For the W > e, we have r_1 = 0, r_2 = 2.3 m (approximate radius of BSMD planes), and B = 0.5 T. With these numbers, you get the simple relation<br> dPhi (cm) = 40 / pT (GeV)<br>For example, an electron of 40 GeV pT will deflect in the phi direction by 1 cm relative to the same e of infinite pT. This is probably good to better than a few %.

  5. run QA : Scott is working on his fills.

no meetings for few weeks

May 21, 2009

Agenda:

  • Joe/Gene - TPC calibration progress, touch upon expected beam line constraint accuracy
  • Rosi/Jan - upgrade of PPV to reconstruct vertex in the transverse plane (for better beam line constraint) diagram, blog from Rosi
  • Scott/Alice (question) - ETOW calibration
  • Willie - correcting BSMD pedestal residual vs. fill , example mod 25, all 120 modules, webpage
    *Joe/Jan - production of L2W-stream could start ~June 15
  • AOB

May 14, 2009

no meeting

May 7, 2009

Present: Gene, Scott, Joe, Jan, Willie, Hal, Dave

  1. TPC:
    • determination of twist & sector alignment in progress, another 10 days needed
    • times of Anode HV on/off will be uploaded to DB in a day
  2. ETOW calib:
    • few dead towers needs to be added to DB
    • slopes from timing scans will be used to determine gains for towers, once Alice will come to IUCF and work on this, in ~10 days.
  3. BTOW: pedestals and status tables uploaded to DB. BTOW status tables done & QAed
  4. Hal run QA comments , spreadsheet PPVEvalBlogPPVEvalBlog
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