Keywords
galaxies: ISM
techniques: spectroscopic
methods: data analysis
Astrophysics - Instrumentation and Methods for Astrophysics
Astrophysics - Astrophysics of Galaxies
techniques: spectroscopic
methods: data analysis
Astrophysics - Instrumentation and Methods for Astrophysics
Astrophysics - Astrophysics of Galaxies
How to Cite
Pipe3D, a pipeline to analyze Integral Field Spectroscopy Data: I. New fitting philosophy of FIT3D. (2016). Revista Mexicana De Astronomía Y Astrofísica, 52(1), 21-53. https://astronomia.unam.mx/journals/rmxaa/article/view/2016rmxaa..52...21s
Abstract
We present an improved version of FIT3D, a fitting tool for the analysis of the spectroscopic properties of the stellar populations and the ionized gas derived from moderate resolution spectra of galaxies. This tool was developed to analyze integral field spectroscopy data and it is the basis of Pipe3D, a pipeline used in the analysis of CALIFA, MaNGA, and SAMI data. We describe the philosophy and each step of the fitting procedure. We present an extensive set of simulations in order to estimate the precision and accuracy of the derived parameters for the stellar populations and the ionized gas. We report on the results of those simulations. Finally, we compare the results of the analysis using FIT3D with those provided by other widely used packages, and we find that the parameters derived by FIT3D are fully compatible with those derived using these other tools.Similar Articles
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