Pixel color-magnitude diagrams of galaxies in the Fornax cluster using S-PLUS images

Galaxy clusters are the largest gravitationally bound systems in the universe and, as such, play an important role in cosmological studies. An important resource for studying their properties in a statistical manner are homogeneous and large image datasets covering diverse environments. In this sens...

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Autores principales: Escudero, Carlos Gabriel, Smith Castelli, Analía Viviana, Faifer, Favio Raúl, Sesto, Leandro Alberto, Mendes de Oliveira, C. L., Herpich, F. R., Barbosa, C. E.
Formato: Articulo
Lenguaje:Inglés
Publicado: 2021
Materias:
Ciencias Astronómicas
surveys
galaxies: clusters: individual (Fornax)
galaxies: photometry
Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/171027
Aporte de:
SEDICI (UNLP) de Universidad Nacional de La Plata
id I19-R120-10915-171027
record_format dspace
spelling I19-R120-10915-1710272024-10-17T16:24:32Z http://sedici.unlp.edu.ar/handle/10915/171027 Pixel color-magnitude diagrams of galaxies in the Fornax cluster using S-PLUS images Escudero, Carlos Gabriel Smith Castelli, Analía Viviana Faifer, Favio Raúl Sesto, Leandro Alberto Mendes de Oliveira, C. L. Herpich, F. R. Barbosa, C. E. 2021 2024-10-02T14:17:31Z en Ciencias Astronómicas surveys galaxies: clusters: individual (Fornax) galaxies: photometry Galaxy clusters are the largest gravitationally bound systems in the universe and, as such, play an important role in cosmological studies. An important resource for studying their properties in a statistical manner are homogeneous and large image datasets covering diverse environments. In this sense, the wide-field images (1.4 deg2) obtained by the Southern Photometric Local Universe Survey (S-PLUS) in 12 optical bands, constitute a valuable tool for that type of studies. In this work, we present a photometric analysis of pixel color-magnitude diagrams, corresponding to a sample of 24 galaxies of different morphological types located in the Fornax cluster. Los cúmulos de galaxias son los sistemas ligados gravitacionalmente más grandes del universo y, como tales, juegan un papel importante en los estudios cosmológicos. Un recurso importante para estudiar sus propiedades de manera estadística es utilizar conjuntos de datos de imágenes homogéneos y de gran cobertura areal que puedan abarcar diversos medioambientes. En este sentido, las imágenes de campo amplio (1.4 grados2) obtenidas por el Southern Photometric Local Universe Survey (S-PLUS) en 12 bandas ópticas, constituyen una valiosa herramienta para ese tipo de estudios. En este trabajo, presentamos un análisis fotométrico de los denominados diagramas color-magnitud pixelados, correspondiente a una muestra de 24 galaxias de diversos tipos morfológicos ubicadas en el cúmulo de Fornax. Asociación Argentina de Astronomía Articulo Articulo http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 174-176
institution Universidad Nacional de La Plata
institution_str I-19
repository_str R-120
collection SEDICI (UNLP)
language Inglés
topic Ciencias Astronómicas
surveys
galaxies: clusters: individual (Fornax)
galaxies: photometry
spellingShingle Ciencias Astronómicas
surveys
galaxies: clusters: individual (Fornax)
galaxies: photometry
Escudero, Carlos Gabriel
Smith Castelli, Analía Viviana
Faifer, Favio Raúl
Sesto, Leandro Alberto
Mendes de Oliveira, C. L.
Herpich, F. R.
Barbosa, C. E.
Pixel color-magnitude diagrams of galaxies in the Fornax cluster using S-PLUS images
topic_facet Ciencias Astronómicas
surveys
galaxies: clusters: individual (Fornax)
galaxies: photometry
description Galaxy clusters are the largest gravitationally bound systems in the universe and, as such, play an important role in cosmological studies. An important resource for studying their properties in a statistical manner are homogeneous and large image datasets covering diverse environments. In this sense, the wide-field images (1.4 deg2) obtained by the Southern Photometric Local Universe Survey (S-PLUS) in 12 optical bands, constitute a valuable tool for that type of studies. In this work, we present a photometric analysis of pixel color-magnitude diagrams, corresponding to a sample of 24 galaxies of different morphological types located in the Fornax cluster.
format Articulo
Articulo
author Escudero, Carlos Gabriel
Smith Castelli, Analía Viviana
Faifer, Favio Raúl
Sesto, Leandro Alberto
Mendes de Oliveira, C. L.
Herpich, F. R.
Barbosa, C. E.
author_facet Escudero, Carlos Gabriel
Smith Castelli, Analía Viviana
Faifer, Favio Raúl
Sesto, Leandro Alberto
Mendes de Oliveira, C. L.
Herpich, F. R.
Barbosa, C. E.
author_sort Escudero, Carlos Gabriel
title Pixel color-magnitude diagrams of galaxies in the Fornax cluster using S-PLUS images
title_short Pixel color-magnitude diagrams of galaxies in the Fornax cluster using S-PLUS images
title_full Pixel color-magnitude diagrams of galaxies in the Fornax cluster using S-PLUS images
title_fullStr Pixel color-magnitude diagrams of galaxies in the Fornax cluster using S-PLUS images
title_full_unstemmed Pixel color-magnitude diagrams of galaxies in the Fornax cluster using S-PLUS images
title_sort pixel color-magnitude diagrams of galaxies in the fornax cluster using s-plus images
publishDate 2021
url http://sedici.unlp.edu.ar/handle/10915/171027
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AT smithcastellianaliaviviana pixelcolormagnitudediagramsofgalaxiesinthefornaxclusterusingsplusimages
AT faiferfavioraul pixelcolormagnitudediagramsofgalaxiesinthefornaxclusterusingsplusimages
AT sestoleandroalberto pixelcolormagnitudediagramsofgalaxiesinthefornaxclusterusingsplusimages
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AT barbosace pixelcolormagnitudediagramsofgalaxiesinthefornaxclusterusingsplusimages
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