The Fornax Cluster through S-PLUS

A.V. SMITH CASTELLI; C.L. MENDES DE OLIVEIRA; F. HERPICH; C.E. BARBOSA; C. ESCUDERO; M. GROSSI; L. SODRÉ; C.R DE BOM; L.J. ZENOCRATTI; M.E. DE ROSSI; A. CORTESI; R. CID FERNANDES; A.R. LOPES; E. TELLES; G.B.O. SCHWARZ; M.L.L DANTAS; F.R. FAIFER; A. CHIES SANTOS; J. SAPONARA; V. REYNALDI; I. ANDRUCHOW; L. SESTO; M.F. MESTRE; A.L. DE AMORIM; E.V.R. DE LIMA; J.C.R. ABBOUD; V. CERNIC; I. SOUZA DE ALMEIDA GARCIA

Rosario

Congreso; 62 Reunión Anual de la Asociación Argentina de Astronomía (edición virtual); 2020

Universidad Nacional de Rosario

The Southern Photometric Local Universe Survey (S-PLUS) aims to map ≈ 9300 deg2 of theSouthern sky using the Javalambre filter system of 12 optical bands, 5 Sloan-like filters and 7 narrow-band filters centered on several prominent stellar features ([OII], Ca H+K, D4000, Hδ, Mgb, Hα and CaT). S-PLUS is carried out with the T80-South, a new robotic 0.826-m telescope located on CTIO, equipped with a wide FoV camera (2 deg^2). In this poster we introduce project #59 of the S-PLUS collaboration aimed at studying the Fornax galaxy cluster covering an sky area of ≈ 11 × 7 deg^2, and with homogeneous photometry in the 12 optical bands of S-PLUS (Coordinator: A. Smith Castelli).