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S-PLUS: LEnticular Galaxies in Stripe 82 (LEGS82).
Cortesi, Arianna; Saha, Kanak; Ferrari, Fabricio; Lucatelli, Geferson; Oliveira, Claudia M DE; Dhiwar, Suraj; Bom, Clecio R; Dias, Luciana Olivia.
Afiliação
  • Cortesi A; Observatório do Valongo (OV), Ladeira do Pedro Antônio 43, Centro, 20080-090 Rio de Janeiro, RJ, Brazil.
  • Saha K; Inter-University Centre for Astronomy and Astrophysics (IUCAA), Post Bag 4, Ganeshkhind, Pune, Maharashtra 411007, India.
  • Ferrari F; Universidade Federal do Rio Grande (FURG), Instituto de Matemática Estatística e Física (IMEF), Av. Itália, km 8, Bairro Carreiros, 96203-900 Rio Grande, RS, Brazil.
  • Lucatelli G; Universidade Federal do Rio Grande (FURG), Instituto de Matemática Estatística e Física (IMEF), Av. Itália, km 8, Bairro Carreiros, 96203-900 Rio Grande, RS, Brazil.
  • Oliveira CM; Departamento de Astronomia, Instituto de Astronomia, Geofísica e Ciências Atmosféricas da USP, Cidade Universitária, 05508-900 São Paulo, SP, Brazil.
  • Dhiwar S; Inter-University Centre for Astronomy and Astrophysics (IUCAA), Post Bag 4, Ganeshkhind, Pune, Maharashtra, 411007, India.
  • Bom CR; Centro Brasileiro de Pesquisas Físicas (CBPF), Rua Dr. Xavier Sigaud 150, Urca, 22290-180 Rio de Janeiro, RJ, Brazil.
  • Dias LO; Centro Brasileiro de Pesquisas Físicas (CBPF), Rua Dr. Xavier Sigaud 150, Urca, 22290-180 Rio de Janeiro, RJ, Brazil.
An Acad Bras Cienc ; 93(suppl 1): e20200989, 2021.
Article em En | MEDLINE | ID: mdl-34008767
ABSTRACT
This work is a Brazilian-Indian collaboration. It aims at investigating the structural properties of Lenticular galaxies in the Stripe 82 using a combination of S-PLUS (Southern Photometric Local Universe Survey) and SDSS data. S-PLUS is a novel optical multi-wavelength survey which will cover nearly 8000 square degrees of the Southern hemisphere in the next years and the first data release covers the Stripe 82 area. The morphological classification and study of the galaxies' stellar population will be performed combining the Bayesian Spectral type (from BPZ) and Morfometryka (MFMTK) parameters. BPZ and MFMTK are two complementary techniques, since the first one determines the most likely stellar population of a galaxy, in order to obtain its photometric redshift (phot-z), and the second one recovers non-parametric morphological quantities, such as asymmetries and concentration. The combination of the two methods allows us to explore the correlation between galaxies shapes (smooth, with spiral arms, etc.) and their stellar contents (old or young population). The preliminary results, presented in this work, show how this novel data set opens a new window on our understanding of the nearby universe.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: An Acad Bras Cienc Ano de publicação: 2021 Tipo de documento: Article

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: An Acad Bras Cienc Ano de publicação: 2021 Tipo de documento: Article