SCALE

About the project

S-PLUS Clusters/Groups and their Large-scale Environments (SCALE) explores how galaxies grow, evolve, and interact within clusters, groups, and the vast cosmic web that connects them. SCALE combines 12-filter optical data with public spectroscopy and high-resolution imaging to reveal the structure and history of galaxies, from dense cluster cores to their outermost regions, extending up to five times the cluster's virial radius.

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Latest publications

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IF6.1Journal Impact Factor from the Journal Citation Reports 2025
AcceptedAccepted for publication, not yet in an issue
S-PLUS Clusters And Large-scale Environments (SCALE): II. PZWav versus redMaPPer identification of eRosita groups
L. Doubrawa, A. Finoguenov, E. S. Cypriano, C. Mendes de Oliveira, E. V. Lima et al.
Astronomy & Astrophysics
IF5.7Journal Impact Factor from the Journal Citation Reports 2025
Recently publishedPublished within the last 6 months
S-PLUS Clusters And Large-scale Environments (SCALE): I. A catalog of known systems in DR5 and a pilot study of Abell 4038
C. Mendes de Oliveira, N. M. Cardoso, P. A. A. Lopes, A. L. B. Ribeiro, D. E. Olave-Rojas et al.
The Astrophysical Journal
1 citationCitations recorded in OpenAlex
IF6.1Journal Impact Factor from the Journal Citation Reports 2025
SCALE: Using S-PLUS photometric information to analyse the brightest cluster galaxy alignment with satellite galaxies
L. Doubrawa, R. Smith, C. Mendes de Oliveira, A. L. O’Mill, L. Nakazono et al.
Astronomy & Astrophysics
2 citationsCitations recorded in OpenAlex

About the project

Research focus

S-PLUS

S-PLUS Clusters And Large-scale Environments (SCALE): II. PZWav versus redMaPPer identification of eRosita groups

S-PLUS Clusters And Large-scale Environments (SCALE): I. A catalog of known systems in DR5 and a pilot study of Abell 4038

SCALE: Using S-PLUS photometric information to analyse the brightest cluster galaxy alignment with satellite galaxies