2022/03/01 by A. V. Smith Castelli, Castelli, A. V. Smith, A. R. Lopes +26
Chemistry · Physics and Astronomy · #Cosmology and Nongalactic Astrophysics (astro-ph.CO) #FOS: Physical sciences #Spectroscopy and Laser Applications #astro-ph.CO
paper · pdf · doi:10.48550/arxiv.2203.00612
3 pages, 5 figures. Accepted to be published in Boletín de la Asociación Argentina de Astronomía
arxiv created 2022/03/01 · openalex publication_date 2022/03/01 · arxiv updated 2022/03/02 · openalex created_date 2022/04/03 · openalex updated_date 2026/08/04
The photometric and morphological analysis of galaxies in clusters provides invaluable information regarding the evolutionary stage of the cluster itself. In addition, it helps to understand how the environment affects the properties of the galaxies and, as a consequence, their evolutionary path. In this contribution we present the first steps on the photometric and morphological analysis of galaxies in the Fornax cluster using S-PLUS data. We expect that the S-PLUS novel filter set and wide field coverage allow us to obtain new information about Fornax and its galaxy population.