Pipe3D, a pipeline for IFS galaxy surveys

We present the most recent results based on Pipe3D, a pipeline tool developed to analysis the spatial resolved stellar population and emission line properties. Previous versions of the pipeline was tested with CALIFA, MaNGA, SAMI and MUSE data (AMUSSING++ compilation), using only one SSP-library (GS...

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Bibliographic Details
Main Authors: Sánchez, Sebastian Francisco, Lacerda, E., Mejía-Narvaez, A., Espinosa-Ponce, C., Lopez, C., Ibarra-Medel, H., Camps-Farina, A., Barrera-Ballesteros, J.K.
Format: Conference Object
Language:unknown
Published: 2021
Subjects:
sami
Online Access:https://zenodo.org/record/4721653
https://doi.org/10.5281/zenodo.4721653
Description
Summary:We present the most recent results based on Pipe3D, a pipeline tool developed to analysis the spatial resolved stellar population and emission line properties. Previous versions of the pipeline was tested with CALIFA, MaNGA, SAMI and MUSE data (AMUSSING++ compilation), using only one SSP-library (GSD156), and a limited set of emission lines (52 galaxies). We introduce a new version of the code fully re-written in Python, that significantly improves the efficiency. In addition we have included different SSP-library analysis and a new set of emission lines (252 in total). We use this new version to analyze the MPL-10 version of the MaNGA dataset (~9500 galaxies), and we are in the process of reanalyzing the AMUSSING++ compilation (~900 galaxies observed with MUSE).

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