S-PLUS: LEnticular Galaxies in Stripe 82 (LEGS82)

Detalhes bibliográficos
Autor(a) principal: CORTESI,ARIANNA
Data de Publicação: 2021
Outros Autores: SAHA,KANAK, FERRARI,FABRICIO, LUCATELLI,GEFERSON, OLIVEIRA,CLAUDIA M. DE, DHIWAR,SURAJ, BOM,CLECIO R., DIAS,LUCIANA OLIVIA
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Anais da Academia Brasileira de Ciências (Online)
Texto Completo: http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0001-37652021000200411
Resumo: 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.
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spelling S-PLUS: LEnticular Galaxies in Stripe 82 (LEGS82)galaxy morphologygalaxy evolutionlenticular galaxiesgalaxy stellar populationfundamental parametersAbstract 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.Academia Brasileira de Ciências2021-01-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersiontext/htmlhttp://old.scielo.br/scielo.php?script=sci_arttext&pid=S0001-37652021000200411Anais da Academia Brasileira de Ciências v.93 suppl.1 2021reponame:Anais da Academia Brasileira de Ciências (Online)instname:Academia Brasileira de Ciências (ABC)instacron:ABC10.1590/0001-3765202120200989info:eu-repo/semantics/openAccessCORTESI,ARIANNASAHA,KANAKFERRARI,FABRICIOLUCATELLI,GEFERSONOLIVEIRA,CLAUDIA M. DEDHIWAR,SURAJBOM,CLECIO R.DIAS,LUCIANA OLIVIAeng2021-06-10T00:00:00Zoai:scielo:S0001-37652021000200411Revistahttp://www.scielo.br/aabchttps://old.scielo.br/oai/scielo-oai.php||aabc@abc.org.br1678-26900001-3765opendoar:2021-06-10T00:00Anais da Academia Brasileira de Ciências (Online) - Academia Brasileira de Ciências (ABC)false
dc.title.none.fl_str_mv S-PLUS: LEnticular Galaxies in Stripe 82 (LEGS82)
title S-PLUS: LEnticular Galaxies in Stripe 82 (LEGS82)
spellingShingle S-PLUS: LEnticular Galaxies in Stripe 82 (LEGS82)
CORTESI,ARIANNA
galaxy morphology
galaxy evolution
lenticular galaxies
galaxy stellar population
fundamental parameters
title_short S-PLUS: LEnticular Galaxies in Stripe 82 (LEGS82)
title_full S-PLUS: LEnticular Galaxies in Stripe 82 (LEGS82)
title_fullStr S-PLUS: LEnticular Galaxies in Stripe 82 (LEGS82)
title_full_unstemmed S-PLUS: LEnticular Galaxies in Stripe 82 (LEGS82)
title_sort S-PLUS: LEnticular Galaxies in Stripe 82 (LEGS82)
author CORTESI,ARIANNA
author_facet CORTESI,ARIANNA
SAHA,KANAK
FERRARI,FABRICIO
LUCATELLI,GEFERSON
OLIVEIRA,CLAUDIA M. DE
DHIWAR,SURAJ
BOM,CLECIO R.
DIAS,LUCIANA OLIVIA
author_role author
author2 SAHA,KANAK
FERRARI,FABRICIO
LUCATELLI,GEFERSON
OLIVEIRA,CLAUDIA M. DE
DHIWAR,SURAJ
BOM,CLECIO R.
DIAS,LUCIANA OLIVIA
author2_role author
author
author
author
author
author
author
dc.contributor.author.fl_str_mv CORTESI,ARIANNA
SAHA,KANAK
FERRARI,FABRICIO
LUCATELLI,GEFERSON
OLIVEIRA,CLAUDIA M. DE
DHIWAR,SURAJ
BOM,CLECIO R.
DIAS,LUCIANA OLIVIA
dc.subject.por.fl_str_mv galaxy morphology
galaxy evolution
lenticular galaxies
galaxy stellar population
fundamental parameters
topic galaxy morphology
galaxy evolution
lenticular galaxies
galaxy stellar population
fundamental parameters
description 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.
publishDate 2021
dc.date.none.fl_str_mv 2021-01-01
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0001-37652021000200411
url http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0001-37652021000200411
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 10.1590/0001-3765202120200989
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv text/html
dc.publisher.none.fl_str_mv Academia Brasileira de Ciências
publisher.none.fl_str_mv Academia Brasileira de Ciências
dc.source.none.fl_str_mv Anais da Academia Brasileira de Ciências v.93 suppl.1 2021
reponame:Anais da Academia Brasileira de Ciências (Online)
instname:Academia Brasileira de Ciências (ABC)
instacron:ABC
instname_str Academia Brasileira de Ciências (ABC)
instacron_str ABC
institution ABC
reponame_str Anais da Academia Brasileira de Ciências (Online)
collection Anais da Academia Brasileira de Ciências (Online)
repository.name.fl_str_mv Anais da Academia Brasileira de Ciências (Online) - Academia Brasileira de Ciências (ABC)
repository.mail.fl_str_mv ||aabc@abc.org.br
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