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[ascl:1907.025] GIST: Galaxy IFU Spectroscopy Tool

GIST (Galaxy IFU Spectroscopy Tool) provides a convenient all-in-one framework for the scientific analysis of fully reduced, (integral-field) spectroscopic data, conducting all the steps from the preparation of input data to the scientific analysis and to the production of publication-quality plots. In its basic set-up, the GIST pipeline extracts stellar kinematics, performs an emission-line analysis, and derives stellar population properties from full spectral fitting and via the measurement of absorption line-strength indices by exploiting pPXF (ascl:1210.002)and GandALF routines. The pipeline is not specific to any instrument or analysis technique, and includes a dedicated visualization routine with a sophisticated graphical user interface for fully interactive plotting of all measurements, spectra, fits, and residuals, as well as star formation histories and the weight distribution of the models.

Code site:
https://abittner.gitlab.io/thegistpipeline/ https://gitlab.com/abittner/gist-development
Described in:
https://ui.adsabs.harvard.edu/abs/2019A%26A...628A.117B
Bibcode:
2019ascl.soft07025B
Preferred citation method:

https://ui.adsabs.harvard.edu/abs/2019A%26A...628A.117B and a footnote linking to https://ascl.net/1907.025


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ascl:1907.025
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