OpenApr 24, 2026
Overdue by 2 month(s)
•Due by February 6, 2026
•Last updated This milestone focuses on adapting WaveDiff for real data processing.
Objectives:
- Add train-test split function to
wf_psf.datapackage (either todata_handler.pyor other module) - Update
SHE_PSF_WaveDiff_Utils/image_processing_utilsmodule with flux normalisation function - Add a dedicated module(s) :
star_select_outlier_removal.pyto thewf_psf.datapackage with method(s) (including helper methods) to perform heavy Central Masking detection and outlier detection (using trained model) and Removal - Parent config file specifying outlier removal methods to execute at run-time
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- Status: Open.#124 In CosmoStat/wf-psf;
- Status: Open.#198 In CosmoStat/wf-psf;
- Status: Open.#199 In CosmoStat/wf-psf;
- Status: Open.#200 In CosmoStat/wf-psf;
- Status: Open.#201 In CosmoStat/wf-psf;
- Status: Open.#207 In CosmoStat/wf-psf;
- Status: Open.#212 In CosmoStat/wf-psf;
- Status: Open (in progress).CosmoStat/wf-psfnumber 213#213 In CosmoStat/wf-psf;