pPXF-SEW: A full-spectrum fitting method of stellar population Synthesis based on ‘’Equivalent Widths spectrum’’ without attenuation curve prior based on pPXF
Description
This pPXF-SEW package contains a Python implementation of the stellar population Synthesis based on Equivalent Widths spectrum (SEW) method and the Penalized PiXel-Fitting (pPXF) method. It uses full-spectrum fitting with SED to extract stellar and gas kinematics, the stellar population, as well as the dust attenuation curve of stars and galaxies, without a prior attenuation curve. The kinematics are derived from the pPXF method, while the stellar population and attenuation curve are derived from the SEW method.
The SEW method was described in Lu (2025).
The pPXF method was originally described in Cappellari & Emsellem (2004) and was substantially upgraded in subsequent years, particularly in Cappellari (2017).
Installation
Install with:
pip install ppxf-sew
Without write access to the global site-packages directory, use:
pip install --user ppxf-sew
To upgrade to the latest version, use:
pip install --upgrade ppxf-sew
Usage Examples
To learn how to use the pPXF-SEW package, run the examples as Jupyter Notebooks in the ppxf-sew/example directory. It can be found within the main pPXF-SEW package installation folder inside site-packages.
License
Other/Proprietary License
Copyright (c) 2024 Jiafeng Lu
This software is provided as is with no warranty. You may use it for non-commercial purposes and modify it for personal or internal use, as long as you include this copyright and disclaimer in all copies. You may not redistribute the code.
1 maintainer
Metadata
1 maintainer
Release files for ppxf-sew 0.8.2
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Total release size: 13.9 MB
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