Difference between revisions of "Fast Offline Analysis Guide"
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− | = Production of DL3 files for a quick-look analysis = | + | = Quick-look next-day analysis = |
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+ | Work in progress... | ||
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+ | Description of the tasks for the fast offline analysis (FOA) | ||
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+ | == Production of DL3 files for a quick-look analysis == | ||
[https://indico.cta-observatory.org/event/5272/contributions/42833/attachments/25228/37023/DL1_to_DL3_basics.pdf Analysis guide] made by Abelardo Moralejo (IFAE) after the [https://indico.cta-observatory.org/event/5272/ LST-1 Analysis 2024 School] | [https://indico.cta-observatory.org/event/5272/contributions/42833/attachments/25228/37023/DL1_to_DL3_basics.pdf Analysis guide] made by Abelardo Moralejo (IFAE) after the [https://indico.cta-observatory.org/event/5272/ LST-1 Analysis 2024 School] | ||
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− | == 1. Selection of the DL1 real data files == | + | === 1. Selection of the DL1 real data files === |
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+ | === 2. Production of the real data DL2 files === | ||
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+ | == Post DL3 analysis == | ||
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+ | === Significance of the detection (theta^2 distribution) === | ||
− | == | + | === 1D spectral analysis === |
Revision as of 09:01, 11 April 2024
Contents
Quick-look next-day analysis
Work in progress...
Description of the tasks for the fast offline analysis (FOA)
Production of DL3 files for a quick-look analysis
Analysis guide made by Abelardo Moralejo (IFAE) after the LST-1 Analysis 2024 School
Outline of the procedure:
1. Start from DL1 files automatically produced by the on-site analysis, LSTOSA (each night's data is typically ready by noon next day)
2. Select the relevant files for a given source, period and zenith distance range
3. Use already existing standard RF models to create DL2 real data files
4. Use the already existing MC test DL2 files (corresponding to the same "production" as the RF models) to create the IRF files
5. Produce the DL3 files