2021/04/27 by Carlos Escudero, C. G. Escudero, A. V. Smith Castelli +14
Environmental Science · Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Astrophysics of Galaxies (astro-ph.GA) #Cluster (spacecraft) #Computer science #FOS: Physical sciences #Fornax Cluster #Galaxies: Formation, Evolution, Phenomena #Galaxy #Galaxy cluster #Homogeneous #Magnitude (astronomy) #Optics #Physics #Pixel #Remote Sensing in Agriculture #Sample (material) #Statistical physics #Universe #astro-ph.GA
paper · pdf · doi:10.48550/arxiv.2104.13496
published in arXiv (Cornell University) (Cornell University) · 3 pages, 4 figures, accepted to be published in Boletin de la Asociacion Argentina de Astronomia
arxiv created 2021/04/27 · openalex publication_date 2021/04/27 · arxiv updated 2021/04/29 · openalex created_date 2021/05/10 · openalex updated_date 2026/07/28
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.