Datasets: Difference between revisions
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* s5 - v576, reconstruct CRV and make analysis ntuples, not uploaded | * s5 - v576, reconstruct CRV and make analysis ntuples, not uploaded | ||
At s1-s4, there is also a truncated data stream, which is | At s1-s4, there is also a truncated data stream, which is events that overflow the SimParticle list. | ||
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| 5/2016 || v576|| sim.mu2e.cd3-cosmic-g4s4-target4.v542_v566_v574_v576.art | | 5/2016 || v576|| sim.mu2e.cd3-cosmic-g4s4-target4.v542_v566_v574_v576.art | ||
|} | |} | ||
==Pions== | ==Pions== | ||
==Antiprotons== | ==Antiprotons== | ||
Revision as of 16:14, 12 September 2017
Beam
Cosmics
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 top gap
- target7 - right top gap
Stages: same as cd3 processing.
6/2017
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. 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.
| date | tag | name |
| 11/2016 | v5-7_9 | sim.mu2e.cd3-cosmic-g4s1-target5.0901a.art |
| 11/2016 | v5-7_9-cosmic-target5-v2 | sim.mu2e.cd3-cosmic-g4s2-target5.1026a_geom1.art |
| 11/2016 | v5-7_9-cosmic-target5-v3 | sim.mu2e.cd3-cosmic-g4s2-target5.1104a_geom2.art |
| 11/2016 | v5-7_9-cosmic-target5-v4 | sim.mu2e.cd3-cosmic-g4s2-target5.1206a_geom3.art |
| 11/2016 | v5-7_9-cosmic-target5-v5 | sim.mu2e.cd3-cosmic-g4s2-target5.1216a_geom4.art |
| 11/2016 | v5-7_9-cosmic-target5-v6 | sim.mu2e.cd3-cosmic-g4s2-target5.1208a_geom5.art |
cd3
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
At s1-s4, 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 |
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. generate and sim to the upstream side of TS1 pbar window. Concatenated dataset sim.mu2e.antiprotons_cs1VD91.170829.art Expert: Bob Bernstein