The GIST pipeline: A multi-purpose tool for the analysis and visualisation of (integral-field) spectroscopic data
The GIST pipeline: A multi-purpose tool for the analysis and visualisation of (integral-field) spectroscopic data
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DOI:
10.1051/0004-6361/201935829
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发表时间:
2019-06
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通讯作者:
A. Bittner;J. Falcón-Barroso;B. Nedelchev;A. Dorta;D. Gadotti;M. Sarzi;Alireza Molaeinezhad;E. Iodice;D. Rosado-Belza;A. D. Lorenzo-Cáceres;F. Fragkoudi;P. M. G. Anta;B. Husemann;J. Méndez-Abreu;J. Neumann;F. Pinna;M. Querejeta;P. Sánchez-Blázquez;M. Seidel
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作者:
A. Bittner;J. Falcón-Barroso;B. Nedelchev;A. Dorta;D. Gadotti;M. Sarzi;Alireza Molaeinezhad;E. Iodice;D. Rosado-Belza;A. D. Lorenzo-Cáceres;F. Fragkoudi;P. M. G. Anta;B. Husemann;J. Méndez-Abreu;J. Neumann;F. Pinna;M. Querejeta;P. Sánchez-Blázquez;M. Seidel
Abstract We introduce the Galaxy IFU Spectroscopy Tool (GIST), a convenient, all-in-one and multi-purpose tool for the analysis and visualisation of already reduced (integral-field) spectroscopic data. In particular, the pipeline performs all steps from read-in and preparation of data to its scientific analysis and visualisation in publication-quality plots. The code measures stellar kinematics and non-parametric star formation histories using the pPXF routine (Cappellari & Emsellem 2004; Cappellari 2017), performs an emission-line analysis with the GandALF procedure (Sarzi et al. 2006; Falcón-Barroso et al. 2006), and determines absorption line-strength indices and their corresponding single stellar population equivalent population properties (Kuntschner et al.2006; Martín-Navarro et al. 2018). The dedicated visualisation routine Mapviewer facilitates the access of all data products in a sophisticated graphical user interface with fully interactive plots.