Difference between revisions of "MC analysis and IRF production"
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The analysis of Monte-Carlo data is mostly done on the cluster in La Palma and the results are accessible in <code> /fefs/aswg/data/mc/ </code> | The analysis of Monte-Carlo data is mostly done on the cluster in La Palma and the results are accessible in <code> /fefs/aswg/data/mc/ </code> | ||
| + | === DL1 === | ||
| + | |||
| + | DL1 MC production to use can be found under: | ||
| + | |||
| + | * <code> /fefs/aswg/data/mc/DL1/20190415/particle/south_pointing/ </code> | ||
| + | |||
| + | Replace particle with gamma, gamma_diffuse, proton or electron. | ||
| + | |||
| + | |||
| + | The dataset is already divided in training/testing for RF production and then IRF production. | ||
| + | |||
| + | Individual DL1 files are merged with parameters only. | ||
| + | |||
| + | |||
| + | === DL2 === | ||
| + | |||
| + | DL2 MC production to use can be found under: | ||
| + | |||
| + | * <code> /fefs/aswg/data/mc/DL1/20190415/particle/south_pointing/ </code> | ||
| + | |||
| + | Replace particle with gamma, gamma_diffuse, proton or electron. | ||
| + | |||
| + | DL2 files are produced from DL1 testing files and corresponding trained RF models. | ||
| + | |||
| + | |||
| + | === RF models === | ||
The trained models to use for data analyse (MC or real data) can be found in <code> /fefs/aswg/data/models/ </code> | The trained models to use for data analyse (MC or real data) can be found in <code> /fefs/aswg/data/models/ </code> | ||
| + | |||
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---- | ---- | ||
| + | == Productions == | ||
=== 23 March 2020 === | === 23 March 2020 === | ||
Revision as of 15:31, 25 March 2020
Contents
Monte-Carlo analysis
The analysis of Monte-Carlo data is mostly done on the cluster in La Palma and the results are accessible in /fefs/aswg/data/mc/
DL1
DL1 MC production to use can be found under:
/fefs/aswg/data/mc/DL1/20190415/particle/south_pointing/
Replace particle with gamma, gamma_diffuse, proton or electron.
The dataset is already divided in training/testing for RF production and then IRF production.
Individual DL1 files are merged with parameters only.
DL2
DL2 MC production to use can be found under:
/fefs/aswg/data/mc/DL1/20190415/particle/south_pointing/
Replace particle with gamma, gamma_diffuse, proton or electron.
DL2 files are produced from DL1 testing files and corresponding trained RF models.
RF models
The trained models to use for data analyse (MC or real data) can be found in /fefs/aswg/data/models/
--Thomas Vuillaume (talk) 16:23, 13 January 2020 (UTC)
Productions
23 March 2020
MC reduction with lstchain v0.4.5 with 2 different configs:
- No intercept
(standard config otherwise)
/fefs/aswg/data/mc/DL2/20190415/***/south_pointing/20200316_v0.4.5__EG1/
/fefs/aswg/data/models/20190415/south_pointing/20200316_v0.4.5__EG1/
- No intercept, no time_gradient
(standard config otherwise)
/fefs/aswg/data/mc/DL2/20190415/***/south_pointing/20200316_v0.4.5__EG2/
/fefs/aswg/data/models/20190415/south_pointing/20200316_v0.4.5__EG2/
02 March 2020
New MC reduction with lstchain v0.4.4 with 3 different configs:
- Standard config:
Cleaning 6-3, LocalPeakWindowSum integrator
/fefs/aswg/data/mc/DL1/20190415/gamma/south_pointing/20200229_v0.4.4_TV01/
/fefs/aswg/data/mc/DL2/20190415/gamma/south_pointing/20200229_v0.4.4_TV01/
/fefs/aswg/data/models/20190415/south_pointing/20200229_v0.4.4_TV01/
- 10p cleaning config:
Cleaning 6.6-3.3, LocalPeakWindowSum integrator
/fefs/aswg/data/mc/DL1/20190415/gamma/south_pointing/20200301_v0.4.4_TV02/
/fefs/aswg/data/mc/DL2/20190415/gamma/south_pointing/20200301_v0.4.4_TV02/
/fefs/aswg/data/models/20190415/south_pointing/20200301_v0.4.4_TV02/
- Neighbor config:
Cleaning 6-3, NeighborPeakWindowSum integrator
/fefs/aswg/data/mc/DL1/20190415/gamma/south_pointing/20200301_v0.4.4_TV03/
/fefs/aswg/data/mc/DL2/20190415/gamma/south_pointing/20200301_v0.4.4_TV03/
/fefs/aswg/data/models/20190415/south_pointing/20200301_v0.4.4_TV03/
--Thomas Vuillaume (talk) 08:44, 2 March 2020 (UTC)
