Pipe3D, a pipeline to analyze integral field spectroscopy data: II. Analysis sequence and CALIFA dataproducts

Titulo: 
Pipe3D, a pipeline to analyze integral field spectroscopy data: II. Analysis sequence and CALIFA dataproducts
Autores: 
Sánchez, S.F., Pérez, E., Sánchez-Blázquez, P., García-Benito, R., Ibarra-Mede, H.J., González, J.J., Rosales-Ortega, F.F., Sánchez-Menguiano, L., Ascasibar, Y., Bitsakis, T., Law, D., Cano-Díaz, M., López-Coba, C., Marino, R.A., De Paz, A.G., López-Sánchez, A.R., Barrera-Ballesteros, J., Galbany, L., Mast, D., Abril-Melgarejo, V., Roman-Lopes, A.
Resumen: 
We present Pipe3D, an analysis pipeline based on the FIT3D fitting tool, developed to explore the properties of the stellar populations and ionized gas of integral field spectroscopy (IFS) data. Pipe3D was created to provide coherent, simple to distribute, and comparable dataproducts, independently of the origin of the data, focused on the data of the most recent IFU surveys (e.g., CALIFA, MaNGA, and SAMI), and the last generation IFS instruments (e.g., MUSE). In this article we describe the different steps involved in the analysis of the data, illustrating them by showing the dataproducts derived for NGC 2916, observed by CALIFA and P-MaNGA. As a practical example of the pipeline we present the complete set of dataproducts derived for the 200 datacubes that comprises the V500 setup of the CALIFA Data Release 2(DR2), making them freely available through the network. Finally, we explore the hypothesis that the properties of the stellar populations and ionized gas of galaxies at the effective radius are representative of the overall average ones, finding that this is indeed the case. © Copyright 2016: Instituto de Astronoḿa, Universidad Nacional Autónoma de México.
Autor principal: 
Sánchez, S.F.
Autor/es del IAA: 
Pérez, E.;García-Benito, R.;Sánchez-Menguiano, L.
Revista: 
Revista Mexicana de Astronomia y Astrofisica
Fecha de publicación: 
2016/04
Volumen: 
52
Issue: 
1
Páginas: 
171-220
Tipo de documento: 
article
Palabras clave: 
Galaxies: structure; Methods: data analysis; Surveys; Techniques: spectroscopic