Pipe3D, a pipeline to analyze integral field spectroscopy data: I. New fitting philosophy of FIT3D
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 PIP...
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ftcsic:oai:digital.csic.es:10261/132991 2024-02-11T10:08:22+01:00 Pipe3D, a pipeline to analyze integral field spectroscopy data: I. New fitting philosophy of FIT3D Sánchez, S.F. Pérez Jiménez, Enrique Barrera-Ballesteros, J 2016-04 http://hdl.handle.net/10261/132991 en eng Universidad Nacional Autónoma de México Publisher's version http://www.astroscu.unam.mx/rmaa/RMxAA.52-1/ Sí Revista Mexicana de Astronomia y Astrofisica 52(1): 21-53 (2016) 0185-1101 http://hdl.handle.net/10261/132991 open galaxies: ISM techniques: spectroscopic artículo http://purl.org/coar/resource_type/c_6501 2016 ftcsic 2024-01-16T10:15:39Z 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. Peer reviewed Article in Journal/Newspaper sami Digital.CSIC (Spanish National Research Council) |
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Digital.CSIC (Spanish National Research Council) |
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ftcsic |
language |
English |
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galaxies: ISM techniques: spectroscopic |
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galaxies: ISM techniques: spectroscopic Sánchez, S.F. Pérez Jiménez, Enrique Barrera-Ballesteros, J Pipe3D, a pipeline to analyze integral field spectroscopy data: I. New fitting philosophy of FIT3D |
topic_facet |
galaxies: ISM techniques: spectroscopic |
description |
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. Peer reviewed |
format |
Article in Journal/Newspaper |
author |
Sánchez, S.F. Pérez Jiménez, Enrique Barrera-Ballesteros, J |
author_facet |
Sánchez, S.F. Pérez Jiménez, Enrique Barrera-Ballesteros, J |
author_sort |
Sánchez, S.F. |
title |
Pipe3D, a pipeline to analyze integral field spectroscopy data: I. New fitting philosophy of FIT3D |
title_short |
Pipe3D, a pipeline to analyze integral field spectroscopy data: I. New fitting philosophy of FIT3D |
title_full |
Pipe3D, a pipeline to analyze integral field spectroscopy data: I. New fitting philosophy of FIT3D |
title_fullStr |
Pipe3D, a pipeline to analyze integral field spectroscopy data: I. New fitting philosophy of FIT3D |
title_full_unstemmed |
Pipe3D, a pipeline to analyze integral field spectroscopy data: I. New fitting philosophy of FIT3D |
title_sort |
pipe3d, a pipeline to analyze integral field spectroscopy data: i. new fitting philosophy of fit3d |
publisher |
Universidad Nacional Autónoma de México |
publishDate |
2016 |
url |
http://hdl.handle.net/10261/132991 |
genre |
sami |
genre_facet |
sami |
op_relation |
Publisher's version http://www.astroscu.unam.mx/rmaa/RMxAA.52-1/ Sí Revista Mexicana de Astronomia y Astrofisica 52(1): 21-53 (2016) 0185-1101 http://hdl.handle.net/10261/132991 |
op_rights |
open |
_version_ |
1790607476576485376 |