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BUDDI-MaNGA I: A statistical sample of cleanly decomposed bulge and disc spectra
Indexado
WoS WOS:000825725300015
Scopus SCOPUS_ID:85135165073
DOI 10.1093/MNRAS/STAC1725
Año 2022
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



Many galaxies display clear bulges and discs, and understanding how these components form is a vital step towards understanding how the galaxy has evolved into what we see today. The BUDDI-MaNGA project aims to study galaxy evolution and morphological transformations through the star-formation histories of the bulges and discs. We have applied our buddi software to galaxies from the MaNGA Survey in the SDSS DR15 in order to isolate their bulge and disc spectra, from which we derived their stellar populations. To date, this work provides the largest sample of clean bulge and disc spectra extracted from IFU datacubes using the galaxies light profile information, and will form the basis for a series of papers aiming to answer open questions on how galaxies have formed and evolved, and the role of their individual structures. This paper presents an introduction to the project, including an overview of these fits, a characterization of the sample, and a series of tests on the fits to ensure reliability.

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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Johnston, Evelyn Mujer Universidad Diego Portales - Chile
2 Häußler, Boris Hombre ESO - Chile
European Southern Observatory Santiago - Chile
European Southern Observ - Chile
3 Jegatheesan, K. - Universidad Diego Portales - Chile

Muestra la afiliación y género (detectado) para los co-autores de la publicación.

Financiamiento



Fuente
FONDECYT
Fondo Nacional de Desarrollo Científico y Tecnológico
Universidad Nacional Autónoma de México
The Ohio State University
Ohio State University
Vanderbilt University
University of Tokyo
Yale University
Alfred P. Sloan Foundation
U.S. Department of Energy Office of Science
University of Arizona
Brazilian Participation Group
Carnegie Mellon University
French Participation Group
Instituto de Astrofisica de Canarias
Johns Hopkins University
Lawrence Berkeley National Laboratory
New Mexico State University
New York University
Pennsylvania State University
University of Portsmouth
University of Utah
University of Virginia
University of Washington
University of Wisconsin-Madison
Office of Science
Max-Planck-Institut fur Extraterrestrische Physik
Carnegie Institution for Science
Chilean Participation Group
Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo
Korean Participation Group
Leibniz Institut fur Astrophysik Potsdam (AIP)
Max-Planck-Institut fur Astronomie (MPIA Heidelberg)
Max-Planck-Institut fur Astrophysik (MPA Garching)
Max-Planck-Institut fur Extraterrestrische Physik (MPE)
National Astronomical Observatories of China
University of Notre Dame
Observatario Nacional/MCTI
Shanghai Astronomical Observatory
United Kingdom Participation Group
University of Colorado Boulder
University of Oxford
University of Wisconsin
Ministerio da Ciencia, Tecnologia e Inovacao
National Astronomical Observatories, Chinese Academy of Sciences
Maritime and Port Authority of Singapore
Center for High Performance Computing at the University of Utah
The Johns Hopkins University
Leibniz-Institut für Astrophysik Potsdam
Max-Planck-Institut fur Astronomie
MPIA Heidelberg
Instituto de Astrof'isica de Canarias
Agencia Nacional de Investigación y Desarrollo
IPMU
Kavli Institute for the Physics and Mathematics of the Universe
Max-Planck-Institut fur Astrophysik
Observatario Nacional
Harvard & Smithsonian
ANID Doctorado Nacional 2021 project
Universidad Nacional Autónoma de México, University of Arizona
ANID Doctorado Nacional 2021 project
Center for Astrophysics, Harvard Smithsonian
Carnegie Mellon University, Center for Astrophysics
Universidad Nacional Autónoma de México, University of Arizona

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics, Harvard & Smithsonian, the Chilean Participation Group, the French Participation Group, Instituto de Astrof ' isica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo, the Korean Participation Group, Lawrence Berkeley National Laboratory, Leibniz Institut fur Astrophysik Potsdam (AIP), Max-Planck-Institut fur Astronomie (MPIA Heidelberg), Max-Planck-Institut fur Astrophysik (MPA Garching), Max-Planck-Institut fur Extraterrestrische Physik (MPE), National Astronomical Observatories of China, New Mexico State University, New York University, University of Notre Dame, Observatario Nacional/MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autonoma de Mexico, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University.
Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions.
SDSS-IV acknowledges support and resources from the Center for High Performance Computing at the University of Utah. The SDSS website is www.sdss.org
SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics, Harvard & Smithsonian, the Chilean Participation Group, the French Participation Group, Instituto de Astrof ' isica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo, the Korean Participation Group, Lawrence Berkeley National Laboratory, Leibniz Institut fur Astrophysik Potsdam (AIP), Max-Planck-Institut fur Astronomie (MPIA Heidelberg), Max-Planck-Institut fur Astrophysik (MPA Garching), Max-Planck-Institut fur Extraterrestrische Physik (MPE), National Astronomical Observatories of China, New Mexico State University, New York University, University of Notre Dame, Observatario Nacional/MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autonoma de Mexico, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University.
We would like to thank the referee for their useful comments which have helped to improve this paper. EJJ acknowledges support from FONDECYT Iniciación en investigación 2020 Project 11200263. KJ acknowledges financial support from ANID Doctorado Nacional 2021 project number 21211770. We gratefully thank the bomberos de Santiago for extinguishing the fire at PUC before it reached the server room where the BUDDI-MANGA data are stored. Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High Performance Computing at the University of Utah. The SDSS website is www.sdss.org . SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, Center for Astrophysics, Harvard & Smithsonian, the Chilean Participation Group, the French Participation Group, Instituto de Astrofísica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU) / University of Tokyo, the Korean Participation Group, Lawrence Berkeley National Laboratory, Leibniz Institut für Astrophysik Potsdam (AIP), Max-Planck-Institut für Astronomie (MPIA Heidelberg), Max-Planck-Institut für Astrophysik (MPA Garching), Max-Planck-Institut für Extraterrestrische Physik (MPE), National Astronomical Observatories of China, New Mexico State Uni versity, Ne w York Uni versity, Uni versity of Notre Dame, Observatário Nacional / MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autónoma de México, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, Uni versity of Virginia, Uni versity of Washington, Uni versity of Wisconsin, Vanderbilt University, and Yale University.

Muestra la fuente de financiamiento declarada en la publicación.