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Summary
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- Released Oct 24, 2019
- 3 contributor(s)
- 7 pull requests
**Description**
*protopipe* 0.2 now fully supports the stable release of *ctapipe* 0.7.0.
The main improvements involve the calibration process
(high gain selected by default),
the direction reconstruction and new camera-type labels.
Code based on *pywi*/*pywi-cta* libraries, relevant for wavelet-based image
cleaning, has been removed in favor of *ctapipe* or made completely optional
where needed. Wavelet cleaning is still optional but will need those two
libraries to be additionally installed. Tailcut-based cleaning is now faster.
The README has been improved with installation, basic use, and developer instructions.
Dependencies are listed in ``protopipe_environment.yaml`` and have been simplified.
The auxiliary scripts ``merge_tables.py`` and ``merge.sh`` have been added to allow merging of DL1 and DL2 HDF5 tables.
The ``mars_cleaning_1st_pass`` method is now imported from _ctapipe_.
Novel code using the largest cluster of survived pixels
(``number_of_islands`` and ``largest_island`` methods in the
``event_preparer`` module) has been hardcoded in _protopipe_ and will
disappear with the next release of _ctapipe_.
Model estimators now load the camera types directly from the ``analysis .yaml`` configuration file.
**Contributors:**
In alphabetical order by first name:
- Alice Donini
- Michele Peresano
- Thierry Stolarczyk
Pull Requests
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This list is incomplete. Small improvements and bug fixes are not listed here.
The complete list is found `here <https://github.com/gammapy/gammapy/pulls?q=is%3Apr+milestone%3A0.16+is%3Aclosed>`__.
- (:pr:`9`) Update image cleaning and make wavelet-based algorithms independent
- (:pr:`8`) Import CTA-MARS 1st pass cleaning from ctapipe