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Searching for codes credited to 'Farrens, S.'

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Found 2 codes.

[ascl:2206.026] ShapePipe: Galaxy shape measurement pipeline
Farrens, S.; Guinot, A.; Kilbinger, M.; Liaudat, T.; Baumont, L.; Jimenez, X.; Peel, A.; Pujol, A.; Schmitz, M.; Starck, J. -L.; Vitorelli, A. Z.
ShapePipe processes single-exposure images and stacked images. Input images have to be calibrated beforehand for astrometry and photometry. The code can handle different image and file types, such as single-exposure mosaic, single-exposure single-CCD, stacked images, database catalog files, and PSF files, some of which are created by the pipeline during the analysis, among others. The end product of ShapePipe is a final catalog containing information for each galaxy, including its shape parameters and the ellipticity components :math:e_1 and :math:e_2. This catalog also contains shapes of artificially sheared images. This information is used in post-processing to compute calibrated shear estimates via metacalibration.
[ascl:2008.005] PySAP: Python Sparse data Analysis Package
Farrens, S.; Grigis, A.; El Gueddari, L.; Ramzi, Z.; Chaithya G. R.; Starck, S.; Sarthou, B.; Cherkaoui, H.; Ciuciu, P.; Starck, J.-L.
PySAP (Python Sparse data Analysis Package) provides a common API for astronomical and neuroimaging datasets and access to iSAP's (ascl:1303.029) Sparse2D executables with both wrappers and bindings. It also offers a graphical user interface for exploring the provided functions and access to application specific plugins.