MDC2018: Difference between revisions

From Mu2eWiki
Jump to navigation Jump to search
 
(27 intermediate revisions by 3 users not shown)
Line 17: Line 17:
* More realistic description of supports, cabling, electronics, etc.
* More realistic description of supports, cabling, electronics, etc.
* Realistic magnetic field map inside the cryostat (Mau13)
* Realistic magnetic field map inside the cryostat (Mau13)
=='''Erratum'''==
The differences in MDC2018b compared to MDC2018a is:
* fix to simulation of panel timing distribution jitter (affects all samples, the importance is under study)
* add CRV output to primaries (affects only primaries)
The difference in MDC2018c compared to MDC2018b is:
* fix fcl so that the ProtonBunchIntensity products is in the output (only effected mixed datasets)
The difference in MDC2018d compared to MDC2018c is:
* fix parentage bug in compression in mixed events (only).  Does not effect primary-only. This fix is in v7_1_2.
The difference in MDC2018e compared to MDC2018d is:
* Improved filling of the end momentum in SimParticle.  This is in v7_1_5.
The difference in MDC2018f compared to MDC2018e is:
* CRV photon simulation uses more efficient 'folded' tables.  Expected changes are <1%.  Switched to v7_2_2
The difference in MDC2018g compared to MDC2018f is:
* Minor bug in CaloShowerStep compression fixed.  No impact on the user as a patch module automatically fixes this when reading older data.  Switched to v7_3_1
The difference in MDC2018h compared to MDC2018g is:
* MCTrajectory for primary particle now saved.  CosmicTimeMap now generated for all primaries.  Switched to v7_4_0
The difference in MDC2018i compared to MDC2018h is:
* A bug in the compression of mixing when applied to pre-digitized and pre-compressed data was fixed.
* A bug in the calculation of the radiation length traversed by a particle going through a straw as reported in TrkStrawHitSeed was fixed.
* MDC2018a-h
** The digi (dig) and reco (mcs) output contains multiple copies of some tracker StepPointMCs.  Workflows that loop over these directly, such as producing mixed digi collections from primary digi collections, will produce erroneous results.  Navigating to tracker StepPointMCs from StrawDigiMCs will produce correct results.
** The radiation length reported by the TrkStraw objects held by the KalSeed objects in the reco dataset is incorrect.  This value was computed for information purposes only, it was not used in the track fit so this bug does not otherwise affect the output.
==Ensemble Datasets==
Fake data ensembles were assembled to mimic what a real dataset from the experiment would look like in order to allow tests of analyses. Details about the production of these ensembles and locations of the datasets can be found [[MDC2018Ensembles | here]].


==Reco Datasets==
==Reco Datasets==
Line 22: Line 58:
Carlo Truth information.  Reco format files occupy less than 1% of the disk space per event as digi files, and
Carlo Truth information.  Reco format files occupy less than 1% of the disk space per event as digi files, and
can be processed more than 1000 times as fast, depending on the job.  Analysis can be run directly on reco datasets.
can be processed more than 1000 times as fast, depending on the job.  Analysis can be run directly on reco datasets.
Only mixed digi samples (Primary Particles with backgrounds) are processed through reconstruction.
Only mixed digi samples (Primary Particles with backgrounds) are processed through reconstruction, and only events
with at least 1 successful Kalman filter fit track (upstream or downstream, electron or muon fit, p>60 MeV/c) are saved.


{|style="width: 90%;text-align:right;"
{|style="width: 90%;text-align:right;"
Line 35: Line 72:
| T ||  7 || 7 || 7350 || 68289 ||  '''mcs.mu2e.CRY-cosmic-general-mix-cat.MDC2018h.art'''
| T ||  7 || 7 || 7350 || 68289 ||  '''mcs.mu2e.CRY-cosmic-general-mix-cat.MDC2018h.art'''
|-
|-
| T ||  5 || 5 || - || - ||  '''mcs.mu2e.CeEndpoint-mix-cat.MDC2018h.art'''
| T ||  25 || 25 || 52815 || 791738 ||  '''mcs.mu2e.CeEndpoint-mix-cat.MDC2018h.art'''
|-
| T ||  25 || 25 || 27105 || 452832 ||  '''mcs.mu2e.CeplusEndpoint-mix-cat.MDC2018h.art'''
|-
| T ||  193 || 193 || 224824 || 3549348 ||  '''mcs.mu2e.flateminus-mix-cat.MDC2018h.art'''
|-
| T ||  25 || 25 || 27747 || 449637 ||  '''mcs.mu2e.flateplus-mix-cat.MDC2018h.art'''
|-
| T ||  13 || 13 || 16326 || 261802 ||  '''mcs.mu2e.flatmugamma-mix-cat.MDC2018h.art'''
|-
| T ||  1 || 1 || 1260 || 19081 ||  '''mcs.mu2e.flatpigamma-mix-cat.MDC2018h.art'''
|-
|-
|}
|}
Line 44: Line 91:
additional simulation or randomness.
additional simulation or randomness.


The differences in MDC2018b compared to MDC2018a is:
* fix to simulation of panel timing distribution jitter (affects all samples, the importance is under study)
* add CRV output to primaries (affects only primaries)
The difference in MDC2018c compared to MDC2018b is:
* fix fcl so that the ProtonBunchIntensity products is in the output (only effected mixed datasets)
The difference in MDC2018d compared to MDC2018c is:
* fix parentage bug in compression in mixed events (only).  Does not effect primary-only. This fix is in v7_1_2.
The difference in MDC2018e compared to MDC2018d is:
* Improved filling of the end momentum in SimParticle.  This is in v7_1_5.
The difference in MDC2018f compared to MDC2018e is:
* CRV photon simulation uses more efficient 'folded' tables.  Expected changes are <1%.  Switched to v7_2_2
The difference in MDC2018g compared to MDC2018f is:
* Minor bug in CaloShowerStep compression fixed.  No impact on the user as a patch module automatically fixes this when reading older data.  Switched to v7_3_1
The difference in MDC2018h compared to MDC2018g is:
* MCTrajectory for primary particle now saved.  CosmicTimeMap now generated for all primaries.  Switched to v7_4_0


===Primary Particles===
===Primary Particles===
Line 137: Line 163:
|-
|-
|    T  ||  4849 ||  4849 || 3555032 ||    738641 ||  '''dig.mu2e.CeplusEndpoint-mix.MDC2018d.art'''
|    T  ||  4849 ||  4849 || 3555032 ||    738641 ||  '''dig.mu2e.CeplusEndpoint-mix.MDC2018d.art'''
|-
|    T  ||  4797 ||  4797 || 2817427 ||    579519 ||  '''dig.mu2e.DS-cosmic-mix.MDC2018d.art'''
|-
|-
|    T  ||  4741 ||  4741 || 4299260 ||    891549 ||  '''dig.mu2e.IPA-Michel-mix.MDC2018d.art'''
|    T  ||  4741 ||  4741 || 4299260 ||    891549 ||  '''dig.mu2e.IPA-Michel-mix.MDC2018d.art'''
Line 678: Line 702:




The following were generated in hash 8c642bc6 (v7_2_0 with new magnetic fields) with fcl taken from the head (see the actual fcl dataset for the final word).
The following were generated in hash 8c642bc6 (v7_2_0 with new magnetic fields) with fcl taken from the head (see the actual fcl dataset for the final word).  DS-cosmic-nofield had Daya Bay generator rate 5494 Hz, so the whole sample, 10M event generated, represents 1820s of livetime.


{|style="width: 90%;text-align:right;"
{|style="width: 90%;text-align:right;"
Line 688: Line 712:
!style="width:10%;text-align:right;"|'''Events'''
!style="width:10%;text-align:right;"|'''Events'''
!style="width:45%;text-align:right;"|'''Dataset'''
!style="width:45%;text-align:right;"|'''Dataset'''
|-|-
|-
|    T  ||    200 ||    200 ||  15411 ||    741357 ||  '''dig.mu2e.CeMLeadingLog.MDC2018e.art'''
|    T  ||    200 ||    200 ||  15411 ||    741357 ||  '''dig.mu2e.CeMLeadingLog.MDC2018e.art'''
|-
|    D  ||    500 ||      0 ||      0 ||          0 ||  cnf.mu2e.DS-cosmic-nofield.MDC2018e.fcl
|    D  ||    500 ||      0 ||      0 ||          0 ||  cnf.mu2e.DS-cosmic-nofield.MDC2018e.fcl
|-
|-
Line 890: Line 915:
|-
|-
|    T  ||    20 ||    20 ||      65 ||          0 ||  bck.mu2e.CRY-cosmic-general-mix.MDC2018g.tbz
|    T  ||    20 ||    20 ||      65 ||          0 ||  bck.mu2e.CRY-cosmic-general-mix.MDC2018g.tbz
|}
The following were generated in v7_5_4 with fcl from the release.
{|style="width: 90%;text-align:right;"
|-
!style="width:10%"|'''Location'''
!style="width:10%;text-align:right;"|'''SAM files'''
!style="width:10%;text-align:right;"|'''Files'''
!style="width:10%;text-align:right;"|'''MB'''
!style="width:10%;text-align:right;"|'''Events'''
!style="width:45%;text-align:right;"|'''Dataset'''
|-
|    D  ||  9846 ||      0 ||      0 ||          0 ||  cnf.mu2e.DS-cosmic-mix.MDC2018i.fcl
|-
|    T  ||      2 ||      2 ||      60 ||          0 ||  bck.mu2e.DS-cosmic-mix.MDC2018i.tbz
|-
|    D  ||    480 ||      0 ||      0 ||          0 ||  cnf.mu2e.DS-cosmic-mix-cat.MDC2018i.fcl
|-
|    T  ||    480 ||    480 || 2728082 ||    578956 ||  '''dig.mu2e.DS-cosmic-mix-cat.MDC2018i.art'''
|-
|    T  ||      4 ||      4 ||      2 ||          0 ||  bck.mu2e.DS-cosmic-mix-cat.MDC2018i.tbz
|}
|}


Latest revision as of 15:06, 30 October 2019

Introduction

A multi-phase production for future studies. The main goals are:

  • Replace the MCStepPoint samples generated for the CD3 review with equivalent samples using updated geometry
  • Provide calibration and analysis samples in 'digi' format
  • Integrate CRV, Calorimeter and Tracker data
  • Provide official samples of signal (mu->e- and mu->e+) and the principal 'faux signal' processes including DIO, cosmic spallation, RMC, RPC
  • Provide 'Mock Data' samples of undifferentiated combinations of signal and faux signal processes, formatted as a high-level skim

MDC2018 samples are intended to facilitate algorithm development, not to support updated precision values of sensitivity or background rates. As such, some approximations are made in the generation compatible with results being accurate at the 90% level.

MDC2018 production started with the CD3 proton-on-target (stage1) output. As such, updates to the production target geometry were not included.

Many updates have been made to the geometry since CD3, including:

  • 21.5mm diameter hole in the stopping target to reduce radiation load on the tracker and STM
  • 18 evenly-spaced Tracker stations with brass shielding interleaved
  • Updated calorimeter crystal sizes and positions
  • More realistic description of supports, cabling, electronics, etc.
  • Realistic magnetic field map inside the cryostat (Mau13)

Erratum

The differences in MDC2018b compared to MDC2018a is:

  • fix to simulation of panel timing distribution jitter (affects all samples, the importance is under study)
  • add CRV output to primaries (affects only primaries)

The difference in MDC2018c compared to MDC2018b is:

  • fix fcl so that the ProtonBunchIntensity products is in the output (only effected mixed datasets)

The difference in MDC2018d compared to MDC2018c is:

  • fix parentage bug in compression in mixed events (only). Does not effect primary-only. This fix is in v7_1_2.

The difference in MDC2018e compared to MDC2018d is:

  • Improved filling of the end momentum in SimParticle. This is in v7_1_5.

The difference in MDC2018f compared to MDC2018e is:

  • CRV photon simulation uses more efficient 'folded' tables. Expected changes are <1%. Switched to v7_2_2

The difference in MDC2018g compared to MDC2018f is:

  • Minor bug in CaloShowerStep compression fixed. No impact on the user as a patch module automatically fixes this when reading older data. Switched to v7_3_1

The difference in MDC2018h compared to MDC2018g is:

  • MCTrajectory for primary particle now saved. CosmicTimeMap now generated for all primaries. Switched to v7_4_0

The difference in MDC2018i compared to MDC2018h is:

  • A bug in the compression of mixing when applied to pre-digitized and pre-compressed data was fixed.
  • A bug in the calculation of the radiation length traversed by a particle going through a straw as reported in TrkStrawHitSeed was fixed.
  • MDC2018a-h
    • The digi (dig) and reco (mcs) output contains multiple copies of some tracker StepPointMCs. Workflows that loop over these directly, such as producing mixed digi collections from primary digi collections, will produce erroneous results. Navigating to tracker StepPointMCs from StrawDigiMCs will produce correct results.
    • The radiation length reported by the TrkStraw objects held by the KalSeed objects in the reco dataset is incorrect. This value was computed for information purposes only, it was not used in the track fit so this bug does not otherwise affect the output.

Ensemble Datasets

Fake data ensembles were assembled to mimic what a real dataset from the experiment would look like in order to allow tests of analyses. Details about the production of these ensembles and locations of the datasets can be found here.


Reco Datasets

These datasets are in 'reco' format : output of the major reconstruction algorithms, with corresponding Monte Carlo Truth information. Reco format files occupy less than 1% of the disk space per event as digi files, and can be processed more than 1000 times as fast, depending on the job. Analysis can be run directly on reco datasets. Only mixed digi samples (Primary Particles with backgrounds) are processed through reconstruction, and only events with at least 1 successful Kalman filter fit track (upstream or downstream, electron or muon fit, p>60 MeV/c) are saved.

Location SAM files Files MB Events Dataset
T 7 7 7350 68289 mcs.mu2e.CRY-cosmic-general-mix-cat.MDC2018h.art
T 25 25 52815 791738 mcs.mu2e.CeEndpoint-mix-cat.MDC2018h.art
T 25 25 27105 452832 mcs.mu2e.CeplusEndpoint-mix-cat.MDC2018h.art
T 193 193 224824 3549348 mcs.mu2e.flateminus-mix-cat.MDC2018h.art
T 25 25 27747 449637 mcs.mu2e.flateplus-mix-cat.MDC2018h.art
T 13 13 16326 261802 mcs.mu2e.flatmugamma-mix-cat.MDC2018h.art
T 1 1 1260 19081 mcs.mu2e.flatpigamma-mix-cat.MDC2018h.art

Digi Datasets

These datasets are in 'digi' format : representations of the detector digital output, with corresponding Monte Carlo truth information. Reconstruction and analysis can be run directly on digi files without additional simulation or randomness.


Primary Particles

Single particle generation, no mixing, with minimal filtering, write out digis and MC products. DS-cosmic were produced using the Daya-Bay generator with DS volume as target, 20K events generated per file, with a generated rate = 5494.24 Hz. Calo-cosmic were also produced using the Daya-Bay generator with the calorimeter disks as target, 20K events generated per file, with a generated rate = 1884.6 Hz.

Location SAM files Files MB Events Dataset
T 250 250 13377 741010 dig.mu2e.flateplus.MDC2018a.art
T 200 200 10546 607985 dig.mu2e.CeplusEndpoint.MDC2018a.art
T 490 490 7485 458118 dig.mu2e.flatmugamma.MDC2018a.art
T 200 200 15807 760512 dig.mu2e.CeEndpoint.MDC2018b.art
T 200 200 51942 1875902 dig.mu2e.IPA-Michel.MDC2018b.art
T 200 200 10175 563481 dig.mu2e.flateminus.MDC2018b.art
T 49230 49230 1675929 44499995 dig.mu2e.DS-cosmic.MDC2018b.art
T 498 498 957 38495 dig.mu2e.flatpigamma.MDC2018b.art
T 10 10 1052 35646 dig.mu2e.proton.MDC2018c.art
T 100 100 14198 102392 dig.mu2e.Calo-cosmic.MDC2018e.art
T 200 200 490 56443 dig.mu2e.flatmugamma-calo.MDC2018e.art
T 500 500 16858 463083 dig.mu2e.DS-cosmic-nofield.MDC2018e.art
T 500 500 24635 179776 dig.mu2e.DS-cosmic-nofield-calo.MDC2018e.art
T 200 200 15411 741357 dig.mu2e.CeMLeadingLog.MDC2018e.art
T 200 200 10197 587822 dig.mu2e.CePLeadingLog.MDC2018e.art
T 500 500 2810 138503 dig.mu2e.flatInternalRPC.MDC2018e.art
T 500 500 21731 1362905 dig.mu2e.flatInternalRMC.MDC2018e.art
T 1952 1952 271367 1999387 dig.mu2e.Calo-cosmic.MDC2018f.art

Primary Particles with background

Single particle generation, with mixing, with minimal filtering, write out digis and MC products. Earlier production versions (MDC2018a-c) had problems and should not be used. The DS-cosmic-mix sample was created by adding background mixing on top of the pure primary events described above.


Location SAM files Files MB Events Dataset
T 972 972 186149 38750 dig.mu2e.flatpigamma-mix.MDC2018d.art
T 4885 4885 2657531 552161 dig.mu2e.flatmugamma-mix.MDC2018d.art
T 4999 4999 4585112 951823 dig.mu2e.CeEndpoint-mix.MDC2018d.art
T 4827 4827 3396206 705688 dig.mu2e.flateplus-mix.MDC2018d.art
T 4849 4849 3555032 738641 dig.mu2e.CeplusEndpoint-mix.MDC2018d.art
T 4741 4741 4299260 891549 dig.mu2e.IPA-Michel-mix.MDC2018d.art
T 38539 38539 26165685 5437807 dig.mu2e.flateminus-mix.MDC2018d.art
T 100 100 506198 102392 dig.mu2e.Calo-cosmic-mix.MDC2018e.art
T 6545 6545 8855370 1868880 dig.mu2e.CRY-cosmic-general-mix.MDC2018g.art

Background only

All backgrounds mixed, no primary particle, no filtering, writing out two datasets: digis and MC products or digis-only (-det).

Location SAM files Files MB Events Dataset
T 198 198 474740 99000 dig.mu2e.NoPrimary-mix.MDC2018d.art
T 198 198 11036 99000 dig.mu2e.NoPrimary-mix-det.MDC2018d.art
T 996 996 2383890 498000 dig.mu2e.NoPrimary-mix.MDC2018e.art
T 996 996 55442 498000 dig.mu2e.NoPrimary-mix-det.MDC2018e.art
T 195 195 2500 4875 dig.mu2e.NoPrimaryFlat-mix-det.MDC2018e.art

Flat Primary Samples

Below is a table of the energy ranges or values used in generating the flat distribution samples described above

Dataset Energy (MeV)
flateminus (-mix) 75 < E < 110
flateplus (-mix) 80 < E < 105
flatmugamma 80 < E < 105
flatmugamma-mix 80 < E < 111
flatpigamma (-mix) 80 < E < 140
CeEndpoint (-mix) E = 104.974
CeplusEndpoint (-mix) E = 92.32

Detailed Datasets

Datasets are presented in the order they were created. The primary dataset that users might be interested in using are in bold. The rest are related to making the main dataset, and are here for the record.

Stopped Particles

These are on cvmfs and can be referred to as "mergedMuonStops/filename" in fcl.

Location SAM files Files MB Events Dataset
T 1 1 14 0 nts.mu2e.DS-IPAstops.MDC2018a.root
T 1 1 302 0 nts.mu2e.DS-OOTstops.MDC2018a.root
T 1 1 129 0 nts.mu2e.DS-TGTstops.MDC2018a.root
T 1 1 421 0 nts.mu2e.pion-DS-TGTstops.MDC2018a.root


CRV flash

The first step is two jobs. The output of cd3 stage 1 was:

  • sim particles from PS to the outside of the CRV (dsregion)
  • sim particles from PS to TS2 (mubeam)

The "PS-CRV" job takes the dsregion sample and propagates it through the CRV. V7_0_0 release.


Location SAM files Files MB Events Dataset
T 25 25 3365 475175 sim.mu2e.PS-CRV-cat.MDC2018a.art
D 2549 0 0 0 cnf.mu2e.PS-CRV.MDC2018a.fcl
T 1 1 0 0 bck.mu2e.PS-CRV-cat.MDC2018a.tbz
T 2548 2548 85471 484298 sim.mu2e.PS-CRV.MDC2018a.art
D 25 0 0 0 cnf.mu2e.PS-CRV-cat.MDC2018a.fcl
T 1 1 99 0 bck.mu2e.PS-CRV.MDC2018a.tbz


The "TS-CRV" job takes the mubeam sample and propagates it through the CRV. V7_0_0 release.


Location SAM files Files MB Events Dataset
T 25 25 44 12175 sim.mu2e.TS-CRV-cat.MDC2018a.art
D 25 0 0 0 cnf.mu2e.TS-CRV-cat.MDC2018a.fcl
T 1 1 196 0 bck.mu2e.TS-CRV.MDC2018a.tbz
T 5092 5092 79442 12408 sim.mu2e.TS-CRV.MDC2018a.art
D 5098 0 0 0 cnf.mu2e.TS-CRV.MDC2018a.fcl
T 1 1 0 0 bck.mu2e.TS-CRV-cat.MDC2018a.tbz
D 5 0 0 0 cnf.mu2e.TS-CRV-cat-cat.MDC2018a.fcl
T 5 5 38 12175 (re-cat) sim.mu2e.TS-CRV-cat-cat.MDC2018a.art
T 1 1 0 0 bck.mu2e.TS-CRV-cat-cat.MDC2018a.tbz

DS

The DS job takes the output of cd3 stage2 (particles traced down the beamline to TS5), and simulates them through the rest of the detector. The CRV StepPoints are written out. The stopped muons in the target and everywhere else are written out to "TGTstops" and "OOTstops". The remainder is written to the "beam" files (which is not used further, the flash is produced in the DS-flash job). Release was v7_0_0.

Location SAM files Files MB Events Dataset
D 5098 0 0 0 cnf.mu2e.DS.MDC2018a.fcl
T 1 1 230 0 bck.mu2e.DS.MDC2018a.tbz
T 25 25 2920 1406275 sim.mu2e.DS-CRV-cat.MDC2018a.art
T 5086 5086 68501 1430463 sim.mu2e.DS-crv.MDC2018a.art
D 25 0 0 0 cnf.mu2e.DS-CRV-cat.MDC2018a.fcl
T 1 1 0 0 bck.mu2e.DS-CRV-cat.MDC2018a.tbz
T 5086 5086 79942 9199955 sim.mu2e.DS-TGTstops.MDC2018a.art
T 5086 5086 103035 20381591 sim.mu2e.DS-OOTstops.MDC2018a.art
T 5086 5086 173850 39742526 sim.mu2e.DS-beam.MDC2018a.art


The stopped muons are produced by running over the art files and writing out ntuples, to be used as input into other jobs. THese are the ntuples:

Location SAM files Files MB Events Dataset
T 1 1 14 0 nts.mu2e.DS-IPAstops.MDC2018a.root
T 1 1 302 0 nts.mu2e.DS-OOTstops.MDC2018a.root
T 1 1 129 0 nts.mu2e.DS-TGTstops.MDC2018a.root

These are also on cvmfs and can be referred to as "mergedMuonStops/filename" in fcl.

Target and Out-Of-Target (OOT) stopped muon products

These jobs take the ntuple of the muons stopped in the target and other locations in the DS (separately) and use them to produce various secondary particles. The release was v7_0_1. Output is StepPoints in the CRV and Trk/Cal separately. Target stop muon decay/capture is modeled using our own physics process algorithms, specific to Al. OOT muon stops are processed by G4, which uses cruder models of the physics but correctly accounts for the heterogenous materials.

Location SAM files Files MB Events Dataset
D 20000 0 0 0 cnf.mu2e.dio.MDC2018a.fcl
T 2 2 125 0 bck.mu2e.dio.MDC2018a.tbz
- 20000 0 0 0 sim.mu2e.dio-CRV.MDC2018a.art
- 20000 0 0 0 sim.mu2e.dio-TrkCal.MDC2018a.art
T 290 290 35608 21802725 sim.mu2e.dio-TrkCal-cat.MDC2018a.art
D 290 0 0 0 cnf.mu2e.dio-TrkCal-cat.MDC2018a.fcl
T 1 1 1 0 bck.mu2e.dio-TrkCal-cat.MDC2018a.tbz
T 290 290 3855 1861571 sim.mu2e.dio-CRV-cat.MDC2018a.art
D 290 0 0 0 cnf.mu2e.dio-CRV-cat.MDC2018a.fcl
T 1 1 1 0 bck.mu2e.dio-CRV-cat.MDC2018a.tbz
D 700 0 0 0 cnf.mu2e.oot.MDC2018a.fcl
- 700 0 0 0 sim.mu2e.oot-TrkCal.MDC2018a.art
- 700 0 0 0 sim.mu2e.oot-CRV.MDC2018a.art
T 1 1 4 0 bck.mu2e.oot.MDC2018a.tbz
T 350 350 2645 2112303 sim.mu2e.oot-TrkCal-cat.MDC2018a.art
D 350 0 0 0 cnf.mu2e.oot-TrkCal-cat.MDC2018a.fcl
T 1 1 1 0 bck.mu2e.oot-TrkCal-cat.MDC2018a.tbz
T 70 70 2628 2112303 (re-cat)sim.mu2e.oot-TrkCal-cat-cat.MDC2018a.art
D 70 0 0 0 cnf.mu2e.oot-TrkCal-cat-cat.MDC2018a.fcl
T 1 1 0 0 bck.mu2e.oot-TrkCal-cat-cat.MDC2018a.tbz
T 350 350 1577 396335 sim.mu2e.oot-CRV-cat.MDC2018a.art
D 350 0 0 0 cnf.mu2e.oot-CRV-cat.MDC2018a.fcl
T 1 1 1 0 bck.mu2e.oot-CRV-cat.MDC2018a.tbz
T 70 70 1556 396335 (re-cat) sim.mu2e.oot-CRV-cat-cat.MDC2018a.art
D 70 0 0 0 cnf.mu2e.oot-CRV-cat-cat.MDC2018a.fcl
T 1 1 0 0 bck.mu2e.oot-CRV-cat-cat.MDC2018a.tbz
D 3500 0 0 0 cnf.mu2e.photon.MDC2018a.fcl
T 1 1 21 0 bck.mu2e.photon.MDC2018a.tbz
- 3500 0 0 0 sim.mu2e.photon-TrkCal.MDC2018a.art
- 3500 0 0 0 sim.mu2e.photon-CRV.MDC2018a.art
T 195 195 47853 34579794 sim.mu2e.photon-TrkCal-cat.MDC2018a.art
D 195 0 0 0 cnf.mu2e.photon-TrkCal-cat.MDC2018a.fcl
T 1 1 0 0 bck.mu2e.photon-TrkCal-cat.MDC2018a.tbz
T 195 195 886 534746 sim.mu2e.photon-CRV-cat.MDC2018a.art
D 195 0 0 0 cnf.mu2e.photon-CRV-cat.MDC2018a.fcl
T 1 1 0 0 bck.mu2e.photon-CRV-cat.MDC2018a.tbz
D 26000 0 0 0 cnf.mu2e.neutron.MDC2018a.fcl
T 3 3 155 0 bck.mu2e.neutron.MDC2018a.tbz
- 26000 0 0 0 sim.mu2e.neutron-CRV.MDC2018a.art
- 26000 0 0 0 sim.mu2e.neutron-TrkCal.MDC2018a.art
T 200 200 59208 14205800 sim.mu2e.neutron-CRV-cat.MDC2018a.art
D 200 0 0 0 cnf.mu2e.neutron-CRV-cat.MDC2018a.fcl
T 1 1 1 0 bck.mu2e.neutron-CRV-cat.MDC2018a.tbz
T 200 200 238025 73789564 sim.mu2e.neutron-TrkCal-cat.MDC2018a.art
D 200 0 0 0 cnf.mu2e.neutron-TrkCal-cat.MDC2018a.fcl
T 1 1 1 0 bck.mu2e.neutron-TrkCal-cat.MDC2018a.tbz
T 50 50 19902 884216 sim.mu2e.deuteron-TrkCal.MDC2018a.art
T 50 50 9 623 sim.mu2e.deuteron-CRV.MDC2018a.art
D 50 0 0 0 cnf.mu2e.deuteron.MDC2018a.fcl
T 1 1 0 0 bck.mu2e.deuteron.MDC2018a.tbz
T 150 150 57645 3030993 sim.mu2e.proton-TrkCal.MDC2018a.art
T 150 150 14 71 sim.mu2e.proton-CRV.MDC2018a.art
D 150 0 0 0 cnf.mu2e.proton.MDC2018a.fcl
T 1 1 0 0 bck.mu2e.proton.MDC2018a.tbz

DS flash

In this job the cd3 stage 2 output (particles at TS5) are propagated through the detector and StepPoints are written out. This job runs over the input sample 20 times to produce a higher-statistics sample of flash in the detector than can be generated in the previous (DS) job. Run in v7_0_2.


Location SAM files Files MB Events Dataset
SD 50980 0 0 0 cnf.mu2e.DS-flash.MDC2018b.fcl
T 6 6 496 0 bck.mu2e.DS-flash.MDC2018b.tbz
- 50980 0 0 0 sim.mu2e.DS-flash-TrkCal.MDC2018b.art
T 255 255 164202 48591244 sim.mu2e.DS-flash-TrkCal-cat.MDC2018b.art
D 255 0 0 0 cnf.mu2e.DS-flash-TrkCal-cat.MDC2018b.fcl
T 2 2 2 0 bck.mu2e.DS-flash-TrkCal-cat.MDC2018b.tbz

Cut Samples

In these jobs, the stepoints that cannot contribute to digis are dropped to greatly decrease the file sizes. The input dataset can be found as the output dataset name without the "-cut". Run in v7_0_4.

Location SAM files Files MB Events Dataset
D 25 0 0 0 cnf.mu2e.PS-CRV-cut.MDC2018a.fcl
T 25 25 589 212127 sim.mu2e.PS-CRV-cut.MDC2018a.art
T 1 1 0 0 bck.mu2e.PS-CRV-cut.MDC2018a.tbz
D 5 0 0 0 cnf.mu2e.PS-CRV-cut-cat.MDC2018a.fcl
T 5 5 586 212127 (re-cat) sim.mu2e.PS-CRV-cut-cat.MDC2018a.art
T 1 1 0 0 bck.mu2e.PS-CRV-cut-cat.MDC2018a.tbz
D 25 0 0 0 cnf.mu2e.DS-CRV-cut.MDC2018a.fcl
T 25 25 22 7294 sim.mu2e.DS-CRV-cut.MDC2018a.art
T 1 1 0 0 bck.mu2e.DS-CRV-cut.MDC2018a.tbz
D 5 0 0 0 cnf.mu2e.DS-CRV-cut-cat.MDC2018a.fcl
T 5 5 18 7294 (re-cat) sim.mu2e.DS-CRV-cut-cat.MDC2018a.art
T 1 1 0 0 bck.mu2e.DS-CRV-cut-cat.MDC2018a.tbz
D 255 0 0 0 cnf.mu2e.DS-flash-TrkCal-cut.MDC2018a.fcl
T 255 255 1415 736713 sim.mu2e.DS-flash-TrkCal-cut.MDC2018a.art
T 1 1 1 0 bck.mu2e.DS-flash-TrkCal-cut.MDC2018a.tbz
D 51 0 0 0 cnf.mu2e.DS-flash-TrkCal-cut-cat.MDC2018a.fcl
T 51 51 1354 736713 (re-cat) sim.mu2e.DS-flash-TrkCal-cut-cat.MDC2018a.art
T 1 1 0 0 bck.mu2e.DS-flash-TrkCal-cut-cat.MDC2018a.tbz

Pion Stops

These were created by William Song and Dave Brown in a private job. The cd3 stage 1 is propagated to the DS and pion stops are written out to an ntuple, uploaded by hand. The fcl used should have been committed.

Location SAM files Files MB Events Dataset
T 1 1 421 0 nts.mu2e.pion-DS-TGTstops.MDC2018a.root

Primary Particles

Single particle generation, no mixing, with minimal filtering, write out digis and MC products. Run in v7_0_5.

Location SAM files Files MB Events Dataset
deleted 200 0 0 0 cnf.mu2e.CeEndpoint.MDC2018a.fcl
deleted 200 200 16167 775750 dig.mu2e.CeEndpoint.MDC2018a.art
deleted 1 1 0 0 bck.mu2e.CeEndpoint.MDC2018a.tbz
deleted 200 0 0 0 cnf.mu2e.flateminus.MDC2018a.fcl
deleted 200 200 12756 676282 dig.mu2e.flateminus.MDC2018a.art
deleted 1 1 0 0 bck.mu2e.flateminus.MDC2018a.tbz
D 250 0 0 0 cnf.mu2e.flateplus.MDC2018a.fcl
T 250 250 13377 741010 dig.mu2e.flateplus.MDC2018a.art
T 1 1 1 0 bck.mu2e.flateplus.MDC2018a.tbz

The following were generated in v7_0_6

Location SAM files Files MB Events Dataset
D 200 0 0 0 cnf.mu2e.CeplusEndpoint.MDC2018a.fcl
T 200 200 10546 607985 dig.mu2e.CeplusEndpoint.MDC2018a.art
T 1 1 0 0 bck.mu2e.CeplusEndpoint.MDC2018a.tbz
D 500 0 0 0 cnf.mu2e.flatmugamma.MDC2018a.fcl
T 490 490 7485 458118 dig.mu2e.flatmugamma.MDC2018a.art
T 1 1 2 0 bck.mu2e.flatmugamma.MDC2018a.tbz

The following were generated in v7_1_1 with fcl taken from the head (see the actual fcl dataset for the final word).

Location SAM files Files MB Events Dataset
D 200 0 0 0 cnf.mu2e.CeEndpoint.MDC2018b.fcl
T 200 200 15807 760512 dig.mu2e.CeEndpoint.MDC2018b.art
T 1 1 1 0 bck.mu2e.CeEndpoint.MDC2018b.tbz
D 200 0 0 0 cnf.mu2e.IPA-Michel.MDC2018b.fcl
T 200 200 51942 1875902 dig.mu2e.IPA-Michel.MDC2018b.art
T 1 1 0 0 bck.mu2e.IPA-Michel.MDC2018b.tbz
D 200 0 0 0 cnf.mu2e.flateminus.MDC2018b.fcl
T 200 200 10175 563481 dig.mu2e.flateminus.MDC2018b.art
T 1 1 0 0 bck.mu2e.flateminus.MDC2018b.tbz
D 50000 0 0 0 cnf.mu2e.DS-cosmic.MDC2018b.fcl
T 49230 49230 1675929 44499995 dig.mu2e.DS-cosmic.MDC2018b.art
T 5 5 931 0 bck.mu2e.DS-cosmic.MDC2018b.tbz
D 500 0 0 0 cnf.mu2e.flatpigamma.MDC2018b.fcl
T 498 498 957 38495 dig.mu2e.flatpigamma.MDC2018b.art
T 2 2 4 0 bck.mu2e.flatpigamma.MDC2018b.tbz
D 10 0 0 0 cnf.mu2e.proton.MDC2018c.fcl
T 10 10 1052 35646 dig.mu2e.proton.MDC2018c.art
T 1 1 0 0 bck.mu2e.proton.MDC2018c.tbz


The following were generated in v7_1_5 with fcl taken from the head (see the actual fcl dataset for the final word).

Location SAM files Files MB Events Dataset
D 100 0 0 0 cnf.mu2e.Calo-cosmic.MDC2018e.fcl
T 100 100 14198 102392 dig.mu2e.Calo-cosmic.MDC2018e.art
T 1 1 1 0 bck.mu2e.Calo-cosmic.MDC2018e.tbz
D 200 0 0 0 cnf.mu2e.flatmugamma-calo.MDC2018e.fcl
T 200 200 490 56443 dig.mu2e.flatmugamma-calo.MDC2018e.art
T 1 1 2 0 bck.mu2e.flatmugamma-calo.MDC2018e.tbz


The following were generated in hash 8c642bc6 (v7_2_0 with new magnetic fields) with fcl taken from the head (see the actual fcl dataset for the final word). DS-cosmic-nofield had Daya Bay generator rate 5494 Hz, so the whole sample, 10M event generated, represents 1820s of livetime.

Location SAM files Files MB Events Dataset
T 200 200 15411 741357 dig.mu2e.CeMLeadingLog.MDC2018e.art
D 500 0 0 0 cnf.mu2e.DS-cosmic-nofield.MDC2018e.fcl
T 500 500 16858 463083 dig.mu2e.DS-cosmic-nofield.MDC2018e.art
T 500 500 24635 179776 dig.mu2e.DS-cosmic-nofield-calo.MDC2018e.art
T 1 1 10 0 bck.mu2e.DS-cosmic-nofield.MDC2018e.tbz

The following were generated in v7_2_1.

Location SAM files Files MB Events Dataset
D 200 0 0 0 cnf.mu2e.CeMLeadingLog.MDC2018e.fcl
T 200 200 15411 741357 dig.mu2e.CeMLeadingLog.MDC2018e.art
T 1 1 1 0 bck.mu2e.CeMLeadingLog.MDC2018e.tbz
D 200 0 0 0 cnf.mu2e.CePLeadingLog.MDC2018e.fcl
T 200 200 10197 587822 dig.mu2e.CePLeadingLog.MDC2018e.art
T 1 1 1 0 bck.mu2e.CePLeadingLog.MDC2018e.tbz
D 500 0 0 0 cnf.mu2e.flatInternalRPC.MDC2018e.fcl
T 500 500 2810 138503 dig.mu2e.flatInternalRPC.MDC2018e.art
T 1 1 2 0 bck.mu2e.flatInternalRPC.MDC2018e.tbz
D 500 0 0 0 cnf.mu2e.flatInternalRMC.MDC2018e.fcl
T 500 500 21731 1362905 dig.mu2e.flatInternalRMC.MDC2018e.art
T 1 1 2 0 bck.mu2e.flatInternalRMC.MDC2018e.tbz


The following were generated in v7_2_2. Calo-cosmic.MDC2018f simply extends the e version above.

Location SAM files Files MB Events Dataset
D 2000 0 0 0 cnf.mu2e.Calo-cosmic.MDC2018f.fcl
T 1952 1952 271367 1999387 dig.mu2e.Calo-cosmic.MDC2018f.art
T 1 1 37 0 bck.mu2e.Calo-cosmic.MDC2018f.fcl

Primary Particles with background

Single particle generation, with mixing, with minimal filtering, writing out digis and MC products. Run in v7_0_5.

Location SAM files Files MB Events Dataset
deleted 5000 0 0 0 cnf.mu2e.CeEndpointMix.MDC2018a.fcl
deleted 4795 4795 4207875 928050 dig.mu2e.CeEndpoint-mix.MDC2018a.art
deleted 1 1 41 0 bck.mu2e.CeEndpointMix.MDC2018a.tbz
deleted 5000 0 0 0 cnf.mu2e.flateplusMix.MDC2018a.fcl
deleted 4914 4914 3307968 728442 dig.mu2e.flateplus-mix.MDC2018a.art
deleted 1 1 39 0 bck.mu2e.flateplusMix.MDC2018a.tbz


The following were generated in v7_1_1 with fcl taken from the head (see the actual fcl dataset for the final word).

Location SAM files Files MB Events Dataset
deleted 5000 0 0 0 cnf.mu2e.flatmugamma-mix.MDC2018b.fcl
deleted 4992 4992 2549437 574986 dig.mu2e.flatmugamma-mix.MDC2018b.art
deleted 1 1 38 0 bck.mu2e.flatmugamma-mix.MDC2018b.tbz
deleted 1000 0 0 0 cnf.mu2e.flatpigamma-mix.MDC2018c.fcl
deleted 993 993 178131 40070 dig.mu2e.flatpigamma-mix.MDC2018c.art
deleted 1 1 11 0 bck.mu2e.flatpigamma-mix.MDC2018c.tbz
deleted 5000 0 0 0 cnf.mu2e.flatmugamma-mix.MDC2018c.fcl
deleted 4993 4993 2548202 574807 dig.mu2e.flatmugamma-mix.MDC2018c.art
deleted 1 1 49 0 bck.mu2e.flatmugamma-mix.MDC2018c.tbz


The following were generated in v7_1_2 with fcl taken from the release or from the head.

Location SAM files Files MB Events Dataset
D 1000 0 0 0 cnf.mu2e.flatpigamma-mix.MDC2018d.fcl
T 972 972 186149 38750 dig.mu2e.flatpigamma-mix.MDC2018d.art
T 1 1 12 0 bck.mu2e.flatpigamma-mix.MDC2018d.tbz
D 5000 0 0 0 cnf.mu2e.flatmugamma-mix.MDC2018d.fcl
T 4885 4885 2657531 552161 dig.mu2e.flatmugamma-mix.MDC2018d.art
T 1 1 48 0 bck.mu2e.flatmugamma-mix.MDC2018d.tbz
D 5000 0 0 0 cnf.mu2e.CeEndpoint-mix.MDC2018d.fcl
T 4999 4999 4585112 951823 dig.mu2e.CeEndpoint-mix.MDC2018d.art
T 2 2 46 0 bck.mu2e.CeEndpoint-mix.MDC2018d.tbz
D 5000 0 0 0 cnf.mu2e.flateplus-mix.MDC2018d.fcl
T 4827 4827 3396206 705688 dig.mu2e.flateplus-mix.MDC2018d.art
T 1 1 44 0 bck.mu2e.flateplus-mix.MDC2018d.tbz
D 5000 0 0 0 cnf.mu2e.CeplusEndpoint-mix.MDC2018d.fcl
T 4849 4849 3555032 738641 dig.mu2e.CeplusEndpoint-mix.MDC2018d.art
T 1 1 55 0 bck.mu2e.CeplusEndpoint-mix.MDC2018d.tbz
D 4923 0 0 0 cnf.mu2e.DS-cosmic-mix.MDC2018d.fcl
T 4797 4797 2817427 579519 dig.mu2e.DS-cosmic-mix.MDC2018d.art
T 1 44 0 0 bck.mu2e.DS-cosmic-mix.MDC2018d.tbz
D 5000 0 0 0 cnf.mu2e.IPA-Michel-mix.MDC2018d.fcl
T 4741 4741 4299260 891549 dig.mu2e.IPA-Michel-mix.MDC2018d.art
T 1 1 56 0 bck.mu2e.IPA-Michel-mix.MDC2018d.tbz
D 40000 0 0 0 cnf.mu2e.flateminus-mix.MDC2018d.fcl
T 38539 38539 26165685 5437807 dig.mu2e.flateminus-mix.MDC2018d.art
T 3 3 253 0 bck.mu2e.flateminus-mix.MDC2018d.tbz


The following were generated in v7_3_4 with fcl modified form the release.

Location SAM files Files MB Events Dataset
D 6545 0 0 0 cnf.mu2e.CRY-cosmic-general-mix.MDC2018g.fcl
T 6545 6545 8855370 1868880 dig.mu2e.CRY-cosmic-general-mix.MDC2018g.art
T 20 20 65 0 bck.mu2e.CRY-cosmic-general-mix.MDC2018g.tbz

The following were generated in v7_5_4 with fcl from the release.

Location SAM files Files MB Events Dataset
D 9846 0 0 0 cnf.mu2e.DS-cosmic-mix.MDC2018i.fcl
T 2 2 60 0 bck.mu2e.DS-cosmic-mix.MDC2018i.tbz
D 480 0 0 0 cnf.mu2e.DS-cosmic-mix-cat.MDC2018i.fcl
T 480 480 2728082 578956 dig.mu2e.DS-cosmic-mix-cat.MDC2018i.art
T 4 4 2 0 bck.mu2e.DS-cosmic-mix-cat.MDC2018i.tbz

Background only

All backgrounds mixed, no primary particle, no filtering, writing out two datasets: digis and MC products or digis-only (-det). Run in v7_0_6.

Location SAM files Files MB Events Dataset
deleted 200 0 0 0 cnf.mu2e.NoPrimary-mix.MDC2018a.fcl
deleted 199 199 439659 99500 dig.mu2e.NoPrimary-mix.MDC2018a.art
deleted 199 199 10915 99500 dig.mu2e.NoPrimary-mix-det.MDC2018a.art
deleted 2 2 1 0 bck.mu2e.NoPrimary-mix.MDC2018a.tbz


The following were generated in v7_1_1 with fcl taken from the head (see the actual fcl dataset for the final word).

Location SAM files Files MB Events Dataset
deleted 200 0 0 0 cnf.mu2e.NoPrimary-mix.MDC2018c.fcl
deleted 199 199 439970 99500 dig.mu2e.NoPrimary-mix.MDC2018c.art
deleted 199 199 10924 99500 dig.mu2e.NoPrimary-mix-det.MDC2018c.art
deleted 2 2 2 0 bck.mu2e.NoPrimary-mix.MDC2018c.tbz


The following were generated in v7_1_2.

Location SAM files Files MB Events Dataset
D 200 0 0 0 cnf.mu2e.NoPrimary-mix.MDC2018d.fcl
T 198 198 474740 99000 dig.mu2e.NoPrimary-mix.MDC2018d.art
T 198 198 11036 99000 dig.mu2e.NoPrimary-mix-det.MDC2018d.art
T 2 2 1 0 bck.mu2e.NoPrimary-mix.MDC2018d.tbz


The following were generated in v7_1_5.

Location SAM files Files MB Events Dataset
D 1000 0 0 0 cnf.mu2e.NoPrimary-mix.MDC2018e.fcl
T 996 996 2383890 498000 dig.mu2e.NoPrimary-mix.MDC2018e.art
T 996 996 55442 498000 dig.mu2e.NoPrimary-mix-det.MDC2018e.art
T 2 2 9 0 bck.mu2e.NoPrimary-mix.MDC2018e.tbz

The following were generated in v7_2_0.

Location SAM files Files MB Events Dataset
D 200 0 0 0 cnf.mu2e.NoPrimaryFlat.MDC2018e.fcl (misnamed)
T 195 195 2500 4875 dig.mu2e.NoPrimaryFlat-mix-det.MDC2018e.art
T 1 1 1 0 bck.mu2e.NoPrimaryFlat.MDC2018e.tbz (misnamed)

Checklist

A checklist of tasks in preparation for MDC2018.

Sign off Responsible Topic Notes
Dave (Louisville) Tracker and OPA Geometry
Bertrand Calorimeter Geometry
Yuri Shielding Geometry
Ralf CRV Geometry
Andy Target and IPA Geometry
?? MBS + STM Geometry
Dave (Louisville) Alignment Infrastructure
Rob/Krzysztof StepPointMC StrawIndex->StrawId
Dave (LBL) Tracker Misalignment
Bertrand Calo Misalignment
Andrei beam fcl
Andrei beam profile
Yuri CRV fcl
Andrei Calo compression
Andrei BG mix fcl
Ray Job Validation
Pasha Radiative DIO weights
Retrieved from "http://mu2ewiki.fnal.gov/w/index.php?title=MDC2018&oldid=14838"