TY - JOUR
T1 - The GIST pipeline: a multi-purpose tool for the analysis and visualisation of (integral-field) spectroscopic data
AU - Bittner, A.
AU - Falcón-Barroso, J.
AU - Nedelchev, B.
AU - Dorta, A.
AU - Gadotti, D. A.
AU - Sarzi, M.
AU - Molaeinezhad, A.
AU - Iodice, E.
AU - Rosado-Belza, D.
AU - De Lorenzo-Cáceres, A.
AU - Fragkoudi, F.
AU - Galán-de Anta, P. M.
AU - Husemann, B.
AU - Méndez-Abreu, J.
AU - Neumann, J.
AU - Pinna, F.
AU - Querejeta, M.
AU - Sánchez-Blázquez, P.
AU - Seidel, M. K.
PY - 2019/6/1
Y1 - 2019/6/1
N2 - 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.
AB - 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.
KW - Methods: data analysis
KW - techniques: spectroscopic
KW - galaxies: kinematics and dynamics
KW - galaxies: stellar content
KW - galaxies: structure
KW - galaxies: individual: NGC 1433
UR - https://www.cambridge.org/core/product/identifier/S1743921319008652/type/journal_article
U2 - 10.1017/S1743921319008652
DO - 10.1017/S1743921319008652
M3 - Article
SN - 1743-9213
VL - 14
SP - 284
EP - 285
JO - Proceedings of the International Astronomical Union
JF - Proceedings of the International Astronomical Union
IS - S353
ER -