Publication info

Title: The S-PLUS Fornax Project (S+FP): A first 12-band glimpse of the Fornax galaxy cluster
Authors: A.V. Smith Castelli, A. Cortesi, R.F. Haack, A.R. Lopes, J. Thainá-Batista, R. Cid Fernandes, L. Lomelí-Núñez, U. Ribeiro, C.R. de Bom, V. Cernic, L. Sodré Jr, L. Zenocratti, M.E. De Rossi, J.P. Calderón, F. Herpich, E. Telles, K. Saha, P.A.A. Lopes, V.H. Lopes-Silva, T.S. Gonçalves, D. Bambrila, N.M. Cardoso, M.L. Buzzo, P. Astudillo Sotomayor, R. Demarco, N. Leigh, M. Sarzi, K. Menéndez-Delmestre, F.R. Faifer, Y. Jiménez-Teja, M. Grossi, J.A. Hernández-Jiménez, A.C. Krabbe, L.A. Gutiérrez Soto, D. Brandão, L. Espinosa, D.E. Olave-Rojas, G.B. Oliveira Schwarz, F. Almeida-Fernandes, W. Schoenell, T. Ribeiro, A. Kanaan, C. Mendes de Oliveira
Publication date: 2024
Journal: Monthly Notices of the Royal Astronomical Society
JIF: 4.8 WoS: 8 Scopus: 6 OpenAlex: 8

Abstract

The Fornax galaxy cluster is the richest nearby (D \(\sim\) 20 Mpc) galaxy association in the southern sky. As such, it provides a wealth of opportunities 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 \(\sim\) 1.4 \(\times\) 1.4 deg\(^2\)) observed in five Sloan Digital Sky Survey-like ugriz broad bands and seven narrow bands covering specific spectroscopic features like [O ii], Ca ii H+K, H\(\delta\), G band, Mg b triplet, H\(\alpha\), and the Ca ii triplet. Based on S-PLUS specific automated photometry, aimed at correctly detecting Fornax galaxies and globular clusters in S-PLUS images, our data set provides the community with catalogues containing homogeneous 12-band photometry for \(\sim 3 \times 106\) resolved and unresolved objects within a region extending over \(\sim\)208 deg\(^2\) (\(\sim\)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\(_\star\) \(\geq\) 108 M\(_\odot\). The S+FP data set we put forward in this first paper of a series will enable a variety of studies some of which are briefly presented.

Citation

@article{castelli2024,
  title = {The {S}-{PLUS} {Fornax} {Project} ({S}+{FP}): {A} first 12-band glimpse of the {Fornax} galaxy cluster},
  volume = {530},
  copyright = {https://creativecommons.org/licenses/by/4.0/},
  issn = {0035-8711, 1365-2966},
  shorttitle = {The {S}-{PLUS} {Fornax} {Project} ({S}+{FP})},
  url = {https://academic.oup.com/mnras/article/530/4/3787/7634368},
  doi = {10.1093/mnras/stae840},
  abstract = {The Fornax galaxy cluster is the richest nearby (D ∼ 20 Mpc) galaxy association in the southern sky. As such, it provides a wealth of opportunities 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 Sloan Digital Sky Survey-like ugriz broad bands and seven narrow bands covering specific spectroscopic features like [O ii], Ca ii H+K, Hδ, G band, Mg b triplet, Hα, and the Ca ii triplet. Based on S-PLUS specific automated photometry, aimed at correctly detecting Fornax galaxies and globular clusters in S-PLUS images, our data set 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 data set we put forward in this first paper of a series will enable a variety of studies some of which are briefly presented.},
  language = {en},
  number = {4},
  urldate = {2025-01-18},
  journal = {Monthly Notices of the Royal Astronomical Society},
  author = {Smith Castelli, A V and Cortesi, A and Haack, R F and Lopes, A R and Thainá-Batista, J and Cid Fernandes, R and Lomelí-Núñez, L and Ribeiro, U and de Bom, C R and Cernic, V and Sodré Jr, L and Zenocratti, L and De Rossi, M E and Calderón, J P and Herpich, F and Telles, E and Saha, K and Lopes, P A A and Lopes-Silva, V H and Gonçalves, T S and Bambrila, D and Cardoso, N M and Buzzo, M L and Astudillo Sotomayor, P and Demarco, R and Leigh, N and Sarzi, M and Menéndez-Delmestre, K and Faifer, F R and Jiménez-Teja, Y and Grossi, M and Hernández-Jiménez, J A and Krabbe, A C and Gutiérrez Soto, L A and Brandão, D and Espinosa, L and Olave-Rojas, D E and Oliveira Schwarz, G B and Almeida-Fernandes, F and Schoenell, W and Ribeiro, T and Kanaan, A and Mendes de Oliveira, C},
  month = may,
  year = {2024},
  pages = {3787--3811},
}