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artículos
Título:
The S-PLUS Fornax Project (S+FP): A first 12-band glimpse of the Fornax galaxy cluster
Autor/es:
CASTELLI, A V SMITH; CORTESI, A; HAACK, R F; LOPES, A R; THAINÁ-BATISTA, J; FERNANDES, R CID; LOMELÍ-NÚÑEZ, L; RIBEIRO, U; DE BOM, C R; CERNIC, V; SODRÉ, L; ZENOCRATTI, L; DE ROSSI, M E; CALDERÓN, J P; HERPICH, F; TELLES, E; SAHA, K; LOPES, P A A; LOPES-SILVA, V H; GONÇALVES, T S; BAMBRILA, D; CARDOSO, N M; BUZZO, M L; SOTOMAYOR, P ASTUDILLO; DEMARCO, R; LEIGH, N; SARZI, M; MENÉNDEZ-DELMESTRE, K; FAIFER, F R; JIMÉNEZ-TEJA, Y; GROSSI, M; HERNÁNDEZ-JIMÉNEZ, J A; KRABBE, A C; SOTO, L A GUTIÉRREZ; BRANDÃO, D; ESPINOSA, L; OLAVE-ROJAS, D E; SCHWARZ, G B OLIVEIRA; ALMEIDA-FERNANDES, F; SCHOENELL, W; RIBEIRO, T; KANAAN, A; DE OLIVEIRA, C MENDES
Revista:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Editorial:
WILEY-BLACKWELL PUBLISHING, INC
Referencias:
Año: 2024
ISSN:
0035-8711
Resumen:
The Fornax galaxy cluster is the richest nearby (D ∼ 20 Mpc) galaxy association in the southern sky. As such, it provides a wealth of oportunities to elucidate on the processes where environment holds a key role in transforming galaxies. Although it has been the focus of many studies, Fornax has never been explored with contiguous homogeneous wide-field imaging in 12 photometric narrow- and broad-bands like those provided by the Southern Photometric Local Universe Survey (S-PLUS). In this paper we present the S-PLUS Fornax Project (S+FP) that aims to comprehensively analyse the galaxy content of the Fornax cluster using S-PLUS. Our data set consists of 106 S-PLUS wide-field frames (FoV∼1.4 ×1.4 deg2) observed in five SDSS-like ugriz broad-bands and seven narrow-bands covering specific spectroscopic features like [OII], CaII H+K, Hδ, G-band, Mg b triplet, Hα, and the CaII triplet. Based on S-PLUS specific automated photometry, aimed at correctly detecting Fornax galaxies and globular clusters in S-PLUS images, our dataset provides the community with catalogues containing homogeneous 12-band photometry for ∼3 × 106 resolved and unresolved objects within a region extending over ∼208 deg2 (∼5 Rvir in RA) around Fornax’ central galaxy, NGC 1399. We further explore the EAGLE and ILLUSTRISTNG cosmological simulations to identify 45 Fornax-like clusters and generate mock images on all 12 S-PLUS bands of these structures down to galaxies with M⋆ ≥ 108 M⊙. The S+FP dataset we put forward in this first paper of a series will enable a variety of studies some of which are briefly presented.