GIST: Galaxy IFU Spectroscopy Tool

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Ada Coda
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GIST: Galaxy IFU Spectroscopy Tool

Post by Ada Coda » Fri Jul 26, 2019 8:57 pm

GIST: Galaxy IFU Spectroscopy Tool

Abstract: 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.

Credit: Bittner, A.; Falcón-Barroso, J.; Nedelchev, B.; Dorta, A.; Gadotti, D. A.; Sarzi, M.; Molaeinezhad, A.; Iodice, E.; Rosado-Belza, D.; de Lorenzo-Cáceres, A.; Fragkoudi, F.; Galán-de Anta, P. M.; Husemann, B.; Méndez-Abreu, J.; Neumann, J.; Pinna, F.; Querejeta, M.; Sánchez-Blázquez, P.; Seidel, M. K.

Site: https://abittner.gitlab.io/thegistpipeline/
https://ui.adsabs.harvard.edu/abs/2019arXiv190604746B

Bibcode: 2019ascl.soft07025B

Preferred citation method: https://ui.adsabs.harvard.edu/abs/2019arXiv190604746B

ID: ascl:1907.025

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