Adam Gibson (University of Toronto)

Slides:



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Presentation transcript:

Before collision data: Cosmic clean-up and cell masking (and Data Quality and monitoring issues) Adam Gibson (University of Toronto) Irene Vichou (U. of Illinois at Urbana-Champaign), Richard Teuscher (IPP/Toronto), Silvia Resconi (Dipartimento di Fisica Milano) ATLAS Hadronic Calibration Workshop; Foz do Arelho; Portugal; June 26, 2009

Roadmap for Validation of ETmiss Before Collisions: Data Quality Noise Dead channels 2009 data: First collisions Surprises in data Minbias Dijets Validation of each term Muon, cryostat Observables 2010 data: 10-100 pb-1 Zee, Zmumu Neutrinofication Ztau tau Wlnu ttbar MET Tails in SUSY (next talk) also Cosmic and single beam backgrounds Online monitoring and DQ Not just ETmiss, but jets, constituents Minbias: no cryo term. QCD: cryo term important 6/20/2018 Hadronic Calibration Workshop Lisbon

Cosmics, Cell masking, Backgrounds, etc. Before collision data: Cosmic clean-up and cell masking (and Data Quality and monitoring issues) Cosmics, Cell masking, Backgrounds, etc. Effect of noise and studies w/ random triggers Cosmics and cleaning cuts Track based ETmiss - potential for background removal Effects of bad calorimeter cells Data Quality and Monitoring CaloMonitoring status and plans Jet/MET Data Quality and monitoring Supplement: Tile commissioning w/ single beams and cosmics

(AG) (LAr) Should follow up the 3-4% disagreement; should be able to get this right! At least for collisions.

Tower jets : multiplicity Investigating jets in random triggers; dependency on jet algorithm March reprocessed commissioning data Standard bad channel masking is applied 60 runs with LAr and Tile (10Sept200823Oct2008) 1.1 million events analyzed Consider only jets satisfying Et > 7 GeV (em-scale) Towers don’t have any noise-suppression Much more jets with seedless algorithms Less jets are found with the ATLAS cone algorithm due to the seed cuts Start a jet if ETtower>1GeV Towers R=0.4 Nikola Makovec

Tower jets (R=0.4) Jets in randomly triggered data are due to: Coherent noise in the barrel PS Problems identified and fixed at hardware level for 2009 data “Sporadic Noise Burst” in the HEC 6 cells which don’t belong to the problematic channels list Jet Occupancy for AntiKt4TowerJets PS HEC Tile Could pick cuts to veto these particular problems in random triggers; but we will need more general cuts (AG) Nikola Makovec

<E>=0.1MeV  Ejet increases by 1GeV Tower jets (R=0.7) The fraction of events with at least one jet with Et>7GeV varies with time. It is correlated with the pedestal shift in the LAr barrel Jet (R=0.7) ~10000cells <E>=0.1MeV  Ejet increases by 1GeV Only 1 set of pedestal values were used to process the data During standard ATLAS running mode, pedestal runs will be daily taken and the database will be modified accordingly. mean energy per cell Nikola Makovec

Noise suppression (AntiKt, R=0.7) Seedless algorithms are infrared-safe but require good understanding of the noise. Inputs to these algorithms should have noise suppression Topoclusters TopoTowers Towers build only with cells belonging to a topocluster Fraction of evts with at least 1 jet (Et>7GeV) Towers : 4.14% Topotowers : 0.04% Topoclusters : 0.05% PS HEC Tile Nikola Makovec

Conclusion The theoretically safe algorithm are more sensitive to the noise since they doesn’t use seed They are also more sensitive to slight pedestal shift Need interaction with detector people For instance, the noise in the barrel PS has been understood and fixed at hard-ware level Looking forward to 2009 data Inputs to these algorithms should have noise suppression Topoclusters or TopoTowers Important to define quality criteria to further remove noisy jets Electromagnetic fraction, energy fraction in presampler,… And also : jet area, fracmax, tracking information, cells Q-factor,… (AG) Should also consider AntiKt, and perhaps other algorithms, for non-random triggers! Will we change the default algorithms in cosmics, as has been discussed for MC09? Nikola Makovec

(AG) And sometimes from detector effects; but MC matches the data reasonably well. Hideki Okawa

Hideki Okawa

Hideki Okawa

Hideki Okawa

Hideki Okawa

Yingchun Zhu

Yingchun Zhu NB: only tile cells considered!

Yingchun Zhu

Yingchun Zhu Adding MB overlay events need not destroy power of cleaning cuts (AG): Caution – it’s not so easy to compare cell times in cosmics and MC. Eventually timing cuts should be very helpful. But, we should make sure it makes sense with the current detectors and cosmics reconstruction.

Yingchun Zhu

B. Meirose

No existing run matches expected LHC conditions. B. Meirose

B. Meirose

B. Meirose We do see “hadronic-only” jets. (AG) Beam halo and beam gas MC seems not very well understood. Normalization unclear (How long is 100k events? What LHC conditions?). Recent improvements in halo MC?

B. Meirose

Require Reject B. Meirose

B. Meirose (AG) More LHC data would help! Important to understand normalization. Less common than cosmics, but beam gas may be harder to veto?

Jackson forLisbon_StoppedGluinos

More details about an interesting analysis, and their background studies with cosmics, on indico. Material: Cosmics as a background to ‘Stopped Gluinos’ L1_J10 trigger planned in empty bunch crossings

(will start by trying to reconstruct the muon!)

Discussion on Cleanup Cuts Many variables under study (Almost?) noone looking at reconstructed muons? Default cuts? “Best” cuts can be analysis dependent Should we propose “One size fits most” cuts? Or just publicize studies, suggest attractive variables, promising cuts? Should we flag suspect events, and leave it to users to ignore them? Or veto suspect events/objects and leave it to special users to recover them? Do we veto events? Or do we consider vetoing/flagging individual clusters, jets, etc? (e.g. calos veto specific cells) Common software tools for applying the cut? Bookkeeping: how to flag suspected “non-collision” events or objects? “Bad event” flag for reporting e.g. LAr data corruption Could it be used for cosmic candidates? Where to implement the cut/search? RAW->ESD? User analysis? Somewhere else? A related question: how to handle jets and EtMiss in the presence of dead regions; Richard will mention again later today

Zhijun cosmicmet2 More about track based MET later today; here a discussion of its use for rejecting non-collision background

Zhijun Liang

Zhijun Liang

` Zhijun Liang

Zhijun Liang

Zhijun Liang

Zhijun Liang

Behi (bumps in MET-phi distribution; phi asymmetry; tile affected cells) LisbonSlides

Behi Fatholahzadeh Define our own “Dead”, “Noisy”, and “Affected” based on detailed LAr categories Tile masks some channels automatically, and all other flagged channels are “Affected” We’re considering the effect of cells flagged, but not corrected, by calos

Before and After EtMiss masking L1Calo Triggers Before and After EtMiss masking First LAr sporadic noise treatment in Easter reprocessing – not included here MET Phi Behi Fatholahzadeh

Behi Fatholahzadeh Energy-dependent phi asymmetry seen in MC; still understanding the comparison with data

“Affected” Delta-MET (103 MeV) “Noisy” MET After Masking (103 MeV) “Bad” Behi Fatholahzadeh

Behi Fatholahzadeh

Conclusions and Plans MET Phi distribution in cosmics being investigated, data and MC Some flagged, but untreated calo cells sometimes have a large effect on EtMiss Especially tile “Affected” cells – identification in process Also LAr SporadicBurstNoise (even after Q event-by-event masking, at least in medium and low gain) Others? Now analyzing March 2009 reprocessing Extend subdetector analysis to full dataset Studying tails of EtMiss distribution Behi Fatholahzadeh

Silvia wrote METCellMaskTool to make these studies easy for EtMiss Are there types of problems the calorimeters should be treating, but aren’t? Are there problems they know about that aren’t even flagged “Affected”? e.g. Tile cells with event-by-event masking – may not be in the DB? Should also understand the efficiency of the masking. (Be prepared for possible remaining problems after CaloCells are built.) Silvia wrote METCellMaskTool to make these studies easy for EtMiss DPD-based, don’t need RAW Should this tool exist for jets also?

Niedercorn (Q and photons) Niedercor.pdf

Q is amplitude dependent: high E -> high Q Fixed in current Tier0 reco Q is amplitude dependent: high E -> high Q Also sensitive to measurement of signal time Saturated cells? F. Niedercorn

(AG) Not so clear how effective the cut is; noone’s tried to calculate the rejection rate? F. Niedercorn

F. Niedercorn Q is hard enough to understand for individual cells; harder for jets and ETMiss Try “photons” first, now requiring a track to improve purity of real cosmics.

F. Niedercorn

See indico for other variables. F. Niedercorn

F. Niedercorn Loose photons should contain more detector effects, fewer cosmics. Can we remove them with Q cut?

(AG) Lots of effort in LAr community towards imagining a better Q factor F. Niedercorn

Discussion on Q and Bad Channels Many possible improvements from subdetectors in using Quality Factor Better LAr Q; tuning sporadicNoise cuts; monitoring; masking of new channels/events, not just known sporadic channels Tile signal quality factor under study, along with OF validation Improvements in LAr Q, E in current reco Now present for medium and low gain cells Potentially significant impact for jets/EtMiss Won’t be present in next (August) reprocessing if it’s done from ESD (decision Wednesday?) Reprocess from RAW, instead? Should Jet/ETMiss raise the point with DPC?

Discussion on Q and Bad Channels If we mask a cell, should we set a flag on the jet, MET, (topo)? Some jet property indicating “OK”, “cleaned”,”suspicious”,”cosmic-like”? MET “significantly affected by channel masking”? What if we think a cell is suspicious, but not masked? Handling of topo clusters – are 0 energy cells (or 1 MeV cells) a problem? Is it important for topo clusters to know about holes (and perhaps skip to the other side?)

Haleh Hadavand

Haleh Hadavand Similar plots for cells, other objects

Haleh Hadavand

Haleh Hadavand

(proposal) If there’s a reason to turn CaloTowers or CaloClusters plots red, it’s also important for jet monitoring and DQ! Haleh Hadavand

JR Lessard

JR Lessard

Jet phi for different blocks of time Consider various levels of MET JR Lessard

JR Lessard

JR Lessard

JR Lessard

JR Lessard

Discussion on DQ Feedback on Jet/EtMiss DQ proposal? Separate METCALO, METMUON flags Inherit non-Green status from the detectors, CaloMon If Jet/EtMiss monitoring shows problems, Yellow (not Red) Do we want online Jet/EtMiss DQ? Or is offline the right place to start? Do we need Jet/EtMiss shifters to look at reprocessed data? What’s the right strategy for imperfect detector coverage? CaloMon DQ status (and plots?) to be reviewed by subdetector and Jet/EtMiss shifters? No separate DQ flag? What triggers, streams, or event selection to use for Jet/EtMiss monitoring?

E)Volpi TileCal? FirstBeamCosmic_v1 Christophe Ochando Ilya Korolkov Tile Calorimeter Performance with calibration, cosmic rays and LHC single beam data E)Volpi TileCal? FirstBeamCosmic_v1 Christophe Ochando Ilya Korolkov Luca Fiorini Matteo Volpi Valerio Rossetti Institut de Física d'Altes Energies Barcelona (Spain) Hadronic calibration workshop 2009 (Lisbon)

-Cosmic data was analyzed to verify the Data Preparation. Introduction -During 2008, 2009 the Tile Calorimeter was commissioned in a series of integration tests with the other ATLAS sub-detectors, trigger and DAQ systems. -Cosmic data was analyzed to verify the Data Preparation. -The commissioning culminated when the Large Hadronic Collider (LHC) circulated proton beams at 450 GeV. Most spectacular: collimator “splash” event in ATLAS “Splash” event in ATLAS 3D display Online monitoring: Atlantis display of cosmic muon event. Runs 87764, Event 40050, Sep 10, 2008 OUTLINE -Timing study with single beam and cosmic events with TileCal -Energy study with single beam events with TileCal -Jet slice algorithms and TileCal with cosmics Matteo Volpi, Hadronic calibration workshop 2009 (Lisbon)

For first beam data the different baselines are due to different Time studies in TileCal with cosmic and splash events Measure of the timing inter-calibration with splash events. Within each partition, an almost flat distribution was observed, demonstrating the very good time equalization performed with laser data, as of the first beam date. EBC LBC LBA EBA TOF Correction EBC LBC LBA EBA For first beam data the different baselines are due to different references. Joao Gentil Direct correlation between cosmic results and beam results. Cosmic cell time response vs beam cell time response both referenced to the time of one channel. Two measurements agree within 2ns on per cell level. EBC LBA Tcosmic LBC EBA Tbeam Matteo Volpi, Hadronic calibration workshop 2009 (Lisbon)

Energy studies in TileCal with scraping events Data taken with the collimator partially closed. Few muons per event passing through TileCal. We measure the response to muons for each partition. No sufficient statistic is available for individual modules. We select muons impacting in the first cells in EBC partition and crossing all Tile until the last cell in EBA partition at the same phi (90deg muons). Most Probable Value of dE/dx signals The average over all cells within a given partition response to horizontal muons is shown for each partition. We verify the inter-calibration of Tile calorimeter cylinders, already calibrated with radioactive gamma sources, down to the 4% precision level. The red lines represent the average MPV value of the 4 barrels and its 4% uncertainty. The average over all cells within a given radial sample response to horizontal muons is shown as function of the radial sample. Colors represent calorimeter response before (blue) and after (red) the per sample corrections to EM scale were applied. Corrections derived from dedicated test beam measurements and Sr radioactive source scans

Monitoring the Jet trigger slice with cosmic events in TileCal Analyzed "jets" that deposited energy in TileCal. Energy correlation plot with fake jets. Correlation plots between the Offline raw energy and the LVL2 uncalibrated energy from October 2008 to May 2009. October 2008 May 2009 Jets in the Long Barrel L2 uncal E [GeV] L2 uncal E [GeV] Jets in the Extended Barrel Offline uncal E [GeV] Offline uncal E [GeV] Important to look at online vs offline energies help to understand the calo trigger performances and debug. Non-diagonal structure in the correlation plots. Problems fixed since December 2008, thanks to a change in the way the energy reconstruction is done at the DSP level in TileCal. Matteo Volpi: Hadronic calibration workshop 2009 (Lisbon)