Datasets: Difference between revisions
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===MDC2018=== | ===MDC2018=== | ||
A | 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. The general goal is to insure the results are accurate at the 80% level. | |||
---- | |||
[[MDC2018 Geometry]] | |||
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) | |||
==Cosmics== | ==Cosmics== | ||
Revision as of 13:45, 23 May 2018
Introduction
This page is an attempt to record the datasets created and uploaded by "production". These are semi-permanent datasets that were created for the collaboration as a whole. It is nearly impossible to maintain dataset information perfectly when any datasets can become invalidated in various ways, or completely obsolete, at any time, for many reasons. Please do not use any datasets without consulting experts in these datasets - that's still the best way to be sure you are using the right dataset.
To print lists of datasets that are known to SAM - all or optionally with restrictions (see -h).
setup mu2efiletools mu2eDatasetList
To see the files in a dataset with full file paths:
mu2eDatasetFileList dataset_name_here >& fcllist.txt
See also Workflows, FileTools and SAM.
Beam
TDR
See TDRDatasets
cd3
See background group.
051017
This sample of stage 1 beam simulation was generated in May 2017 to answer questions about CRV shielding. Default geometry. This sample is standard enough that it could be of use to other groups. Goals of this effort:
- Rates and dead-time with improved precision
- Sources of coincidences from neutrons and gammas
- Improved shielding and CRV geometry to mitigate rates and to increase CRV coverage (geometry changed in later stages)
The standard cd3 beam stage 1 fcl was modified to only write out the dsregion and mubeam datasets. Run in v6_2_1. See 8627 and 7040. Expert: Yuri Oksuzian.
- 500K jobs of 10K POT, total 5e9 POT
- cnf.mu2e.cd3-beam-g4s1.051017.fcl
- sim.mu2e.cd3-beam-g4s1cat-mubeam.051017.art (concatenated 20-to-1, uploaded)
- sim.mu2e.cd3-beam-g4s1cat-dsregion.051017.art (concatenated 20-to-1, uploaded)
geant4 v10 test samples
Run 11/2016 to 2/2017 to test geant4 v10. See doc-9336 doc-9624 doc-9402 doc-9139 doc-8357. For dataset details, see GeantV10Test. Expert: Ray Culbertson and Yuri Oksuzian.
MDC2018
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. The general goal is to insure the results are accurate at the 80% level.
MDC2018 Geometry 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)
Cosmics
Calibration Cosmic Test Sample
Calibration cosmics are events taken with a simulated trigger intended to collect all cosmics that hit a detector, for use in calibration studies. The digis for trk and cal are written out, as well as the StepPointMC's for CRV (the CRV product is being updated). Expert: Ray Culbertson
3/2018, three samples were generated, 1M events generated for each then some filtering.
- ext - detector extracted to +14m in z
- Bfield is on but the default maps do not reach that far, so Bfield appears off
- trigger on trk OR cal
- Dataset: sim.mu2e.cosmic_calib_ext.180302.art
- geometry: Mu2eG4/geom/geom_common_garage.txt (mods to Mu2eG4/geom/geom_common_current.txt)
- Total cosmic rate = 1989.85 Hz for 1M events = 502s livetime
- ins - detect in normal inserted position
- Bfield on
- trigger on trk OR cal
- Dataset: sim.mu2e.cosmic_calib_ins.180302.art
- geometry: Mu2eG4/geom/geom_common.txt (->Mu2eG4/geom/geom_common_cd3_s4p2.txt)
- Total cosmic rate = 1989.85 Hz for 1M events = 502s livetime
- crv - detect in normal inserted position
- Bfield on
- trigger on CRV hits
- Dataset: sim.mu2e.cosmic_calib_crv.180302.art
- geometry: Mu2eG4/geom/geom_common.txt (->Mu2eG4/geom/geom_common_cd3_s4p2.txt)
- Total cosmic rate = 23010.7 Hz for 1M events = 43s livetime
target6/7 Study
Generated to study how cosmics enter the gap between the CRV top and sides, to help determine the CRV final design. Daya Bay generator. Summary talk 11147. Expert: Ralf Ehrlich.
- target6 - left (+x) top gap
- target7 - right (-x) top gap
Stages: same as cd3 processing.
6/2017 full listing
target5 Study
Generated to study cosmic rays that enter the TS hole and produce tracks, and how they can be degraded with new shielding blocks. This follows up on this category of events discovered in CD3 target1. Daya Bay generator. Talk summary 8322. Expert: Ray Culbertson.
The talk shows the various shielding configurations and concludes new shielding would help. Stages:
- s1 - v579, generate on a plane that is the TS opening, sim to a surface between TS3 and TS5
- s2 - various branches off of v579, complete sim, reco, require a track 50-200 MeV.
The job were run around 11/2016.
| git tag | dataset name |
| v5-7_9 | sim.mu2e.cd3-cosmic-g4s1-target5.0901a.art |
| v5-7_9-cosmic-target5-v2 | sim.mu2e.cd3-cosmic-g4s2-target5.1026a_geom1.art |
| v5-7_9-cosmic-target5-v3 | sim.mu2e.cd3-cosmic-g4s2-target5.1104a_geom2.art |
| v5-7_9-cosmic-target5-v4 | sim.mu2e.cd3-cosmic-g4s2-target5.1206a_geom3.art |
| v5-7_9-cosmic-target5-v5 | sim.mu2e.cd3-cosmic-g4s2-target5.1216a_geom4.art |
| v5-7_9-cosmic-target5-v6 | sim.mu2e.cd3-cosmic-g4s2-target5.1208a_geom5.art |
Stage1 fcl and archive:
bck.mu2e.cd3-cosmic-g4s1-target5.0901a.tbz cnf.mu2e.cd3-cosmic-g4s1-target5.0901a.fcl
Stage 2 fcl and archive. The geometry was changed by running the same fcl but a different release, defined by the tag and loaded on cvmfs in OfflineSpecial
cnf.mu2e.cd3-cosmic-g4s2-target5.0901a_geom1.fcl bck.mu2e.cd3-cosmic-g4s2-target5.1026a_geom1.tbz bck.mu2e.cd3-cosmic-g4s2-target5.1104a_geom2.tbz bck.mu2e.cd3-cosmic-g4s2-target5.1206a_geom3.tbz bck.mu2e.cd3-cosmic-g4s2-target5.1216a_geom4.tbz bck.mu2e.cd3-cosmic-g4s2-target5.1208a_geom5.tbz
cd3 background
Produced to determine the cosmic background for CD3 review. Daya Bay generator. Talk summary 7131, memo 3059. Expert: Ralf Ehrlich.
- general - all cosmics passing through a horizontal surface through detector.
- target1 - left side, around TS entrance
- target2 - upstream face
- target3 - downstream face
- target4 - cryo hole
Stages (s1-s4 uploaded)
- s1 - v542, simulate CRV, require 45 MeV of energy on detector volume surface, stop
- s2 - v566, simulate detectors, require 15 straw hits
- s3 - v574, reco, require a track 50-200 MeV
- s4 - v576, require tracks, 100-110 MeV, passing all cuts, PID, no upstream track
- s5 - v576, reconstruct CRV and make analysis ntuples (not uploaded)
For s1 and s2, there is also a truncated data stream, which is events that overflow the SimParticle list.
| date | Offline | name |
| 5/2016 | v576 | sim.mu2e.cd3-cosmic-g4s4-general.v542_v566_v574_v576.art |
| 5/2016 | v576 | sim.mu2e.cd3-cosmic-g4s4-target1.v542_v566_v574_v576.art |
| 5/2016 | v576 | sim.mu2e.cd3-cosmic-g4s4-target2.v542_v566_v574_v576.art |
| 5/2016 | v576 | sim.mu2e.cd3-cosmic-g4s4-target3.v542_v566_v574_v576.art |
| 5/2016 | v576 | sim.mu2e.cd3-cosmic-g4s4-target4.v542_v566_v574_v576.art |
There is another page with a full list of these datasets.
Pions
Antiprotons
Bernstein Study
9/2017 generating antiprotons in the primary target, flat in energy and phase space. head of branch pbarAnalysis, from head after v6_2_3, on Aug 25 15:22, hash 2ce1246d3d7833bcdd8fcf38bcea3ab6f3255755. 100K jobs x 500K pbars, first NERSC production - docker image mu2e/prd:pbar-00. generate and sim to the upstream side of TS1 pbar window. Production: Ray Culbertson, Physics: Bob Bernstein.
- fcl dataset: cnf.rhbob.NERSCprod1.pbarAnalysis_0_1.fcl
- Concatenated dataset (485 files, 177637185 events): sim.mu2e.antiprotons_cs1VD91.170829.art
- logs and TFileService: bck.mu2e.NERSCprod1.170829.tbz