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Generalise table preprocessing #2791
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6605589
test
1a68509
first working version, ruff
0791398
adding/fixing tests, ruff
473c0a1
ruff
298dc02
updating docs
9aaba99
fix the docs, ruff
8042312
addressing sonarqube, ruff
5d7b24b
addressing review, ruff
c07cb52
modifying renaming functionality
44a66a9
Improving changelog
2ca592e
Improving changelog
9042d95
Removing disable_column_renaming
4661647
addressing review
dd4902a
simpifying the table construction
42f58d2
addressing review
36f3eeb
relocating preprocessing to io
d035775
fixing docs and circular imports
40d9f50
fixing tests
15396e3
fixing import that strangely wasn't caught by the tests
ccd427b
trying to fix the minimal dependencies issue
8c924fa
Revert "trying to fix the minimal dependencies issue"
mexanick fb5f8ea
moving all tests that implicitly use pyirf to irf
7f3a16c
removing duplicated lines
5d07e5a
Make pyirf dependency optional, fix dl2_tables_preprocessing exposure
mexanick 802319d
resolving conflicts
9af99dd
Fix min tests for preprocessing
mexanick 4a234a6
Remove "u.dimensionless_unscaled" units from gh_score and weights.
mexanick 7d4960d
fix test fixture (new order of columns)
mexanick e9a17ca
improving the help of a config parameter
1fa7012
supported pointing frames
6bfc371
Variable names, warning, imports
fed7c7f
Variable names, warning, imports
4061c9d
Put annotation when needed by the new importing scheme
11d98e2
Reverting to correct exception
e94ac42
Merge branch 'main' into generalise_table_preprocessing
maxnoe d685e25
Merge remote-tracking branch 'origin/main' into generalise_table_prep…
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| Original file line number | Diff line number | Diff line change |
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| @@ -0,0 +1,3 @@ | ||
| Currently, for telescope cross calibration we have implemented our own table filtering. However similar functionality has been implemented in IRF tools. Our idea is to reuse the existing functionality from IRF tools for cross calibration. The added benefits is increased maintainability. Moreover, cross calibration memory efficiency will be improved by reading data by chunks. Finally, this can potentially benefit other usecases that load DL2 tables. | ||
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| In order to do that, we will propose some modifications in irf/preprocessing. However we should ensure that the default behaviour stays the same. | ||
This file contains hidden or bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
| Original file line number | Diff line number | Diff line change |
|---|---|---|
| @@ -0,0 +1,3 @@ | ||
| Currently, for telescope cross calibration we have implemented our own table filtering. However similar functionality has been implemented in IRF tools. Our idea is to reuse the existing functionality from IRF tools for cross calibration. The added benefits is increased maintainability. Moreover, cross calibration memory efficiency will be improved by reading data by chunks. Finally, this can potentially benefit other usecases that load DL2 tables. | ||
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| In order to do that, we will propose some modifications in irf/preprocessing. However we should ensure that the default behaviour stays the same. |
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