CC BY 4.0HerpichFR Almeida-FernandesF SchwarzGBO LimaEVR NakazonoL Alonso-GarcíaJ Fonseca-FariaMA SartoriMJ BolutaviciusGF de SouzaGF HartmannEA LiL EspinosaL KanaanA SchoenellW WerleA Machado-PereiraE Gutiérrez-SotoLA Santos-SilvaT CastelliAV LacerdaEAD BarbosaCL PerottoniHD LopesCEF ValençaRR MarthoPAR BomCR BonattoCJ CarvalhoMS CernicV FernandesRC CoelhoP CortesiA PalmaBC DoubrawaL AlbericeVSF Quispe-HuaynasiF PerinGJ ArancibiaMJ KrabbeA Lima-DiasC Lomelí-NúñezL de OliveiraRL LopesAR FigueiredoAL LöschE NavareteF OliveiraJM OverzierR PlaccoVM RoigFV RubetM SantosA SasseVH Thainá-BatistaJ Torres-FloresS BeersTC Alvarez-CandalA AkrasS PandaS LimbergG CastellónJLN TellesE LopesPAA MontaguthGDP SilvaLBE HumirePK FernandesMB CordeiroV RibeiroT de OliveiraCMCarlos Ferreira Lopes2025-06-052025-06-0520240004-6361https://hdl.handle.net/20.500.12740/22688Context. The Southern Photometric Local Universe Survey (S-PLUS) is a project to map similar to 9300 sq deg of the sky using twelve bands (seven narrow and five broadbands). Observations are performed with the T80-South telescope, a robotic telescope located at the Cerro Tololo Observatory in Chile. The survey footprint consists of several large contiguous areas, including fields at high and low galactic latitudes, and towards the Magellanic Clouds. S-PLUS uses fixed exposure times to reach point source depths of about 21 mag in the griz and 20 mag in the u and the narrow filters. Aims. This paper describes the S-PLUS Data Release 4 (DR4), which includes calibrated images and derived catalogues for over 3000 sq deg, covering the aforementioned area. The catalogues provide multi-band photometry performed with the tools DoPHOT and SExtractor - point spread function (PSF) and aperture photometry, respectively. In addition to the characterization, we also present the scientific potential of the data. Methods. We use statistical tools to present and compare the photometry obtained through different methods. Overall we find good agreement between the different methods, with a slight systematic offset of 0.05 mag between our PSF and aperture photometry. We show that the astrometry accuracy is equivalent to that obtained in previous S-PLUS data releases, even in very crowded fields where photometric extraction is challenging. The depths of main survey (MS) photometry for a minimum signal-to-noise ratio S/N = 3 reach from similar to 19.5 for the bluer bands to similar to 21.5 mag on the red. The range of magnitudes over which accurate PSF photometry is obtained is shallower, reaching similar to 19 to similar to 20.5 mag depending on the filter. Based on these photometric data, we provide star-galaxy-quasar classification and photometric redshift for millions of objects. Results. We demonstrate the versatility of the data by presenting the results of a project to identify members of four Abell galaxy clusters in the Local Universe. The S-PLUS DR4 data allow for a reliable assessment of cluster membership out to a large radius corresponding to 5 x r(200). The S-PLUS DR4 can be accessed through the survey data portal. All the software used to generate the catalogues for this release and the scientific investigation presented is available in the collaboration GitHub repository. Conclusions. The S-PLUS DR4 consists of a large, calibrated public dataset, providing powerful ways for studying Galactic and extra-galactic objects through an extensive set of (broad and narrow) filters. C1 [Herpich, F. R.] Univ Cambridge, Inst Astron, Cambridge Survey Astron Unit CASU, Madingley Rd, Cambridge CB3 0HA, England. [Almeida-Fernandes, F.; Schwarz, G. B. Oliveira; Lima, E. V. R.; Nakazono, L.; Sartori, M. J.; Bolutavicius, G. F.; de Souza, G. Fabiano; Li, L.; Espinosa, L.; Santos-Silva, T.; Lacerda, E. A. D.; Valenca, R. R.; Martho, P. A. Re; Carvalho, M. S.; Cernic, V.; Coelho, P.; Doubrawa, L.; Alberice, V. S. Ferreira; Krabbe, A.; Figueiredo, A. Luiz; Losch, E.; Oliveira, J. M.; Limberg, G.; Humire, P. K.; de Oliveira, C. Mendes] Inst Astron Geofis & Ciencias Atmosfer, Rua Matao 1226,Cidade Univ, BR-05508090 Sao Paulo, Brazil. [Almeida-Fernandes, F.; Cortesi, A.; Lomeli-Nunez, L.; Rubet, M.; Lopes, P. A. A.] Observ Valongo, Ladeira Pedro Antonio 43, BR-20080090 Rio De Janeiro, Brazil. [Schwarz, G. B. Oliveira; Alberice, V. S. Ferreira] Univ Presbiteriana Mackenzie, Rua Consolacao 930, BR-01302907 Sao Paulo, Brazil. [Nakazono, L.] Univ Washington, 1415 NE 45th St, Seattle, WA 98195 USA. [Alonso-Garcia, J.] Univ Antofagasta, Ctr Astron CITEVA, Av Angamos 601, Antofagasta 1240000, Chile. [Alonso-Garcia, J.; Lopes, C. E. Ferreira] Millennium Inst Astrophys, Nuncio Monsenor Sotero Sanz 100,Of 104, Providencia 7500000, Chile. 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C3 University of Cambridge; University of Washington; University of Washington Seattle; Universidad de Antofagasta; Instituto de Astrofisica de Canarias; Universidade Federal de Santa Catarina (UFSC); University of Padua; Istituto Nazionale Astrofisica (INAF); National University of La Plata; Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET); National University of La Plata; Centro Universitario da FEI; Polish Academy of Sciences; Nicolaus Copernicus Astronomical Center of the Polish Academy of Sciences; Universidad de Atacama; Centro Brasileiro de Pesquisas Fisicas; Centro Federal de Educacao Tecnologica Celso Suckow da Fonseca (CEFET-RJ); Universidade Federal do Rio Grande do Sul; Universidad de La Serena; Universidade de Sao Paulo; Universidad de La Serena; Universidade Federal de Sergipe; Leiden University; Leiden University - Excl LUMC; Netherlands Organization Applied Science Research; National Science Foundation (NSF); National Observatory of Athens; University of Arizona; University of Arizonainfo:eu-repo/semantics/openAccesscatalogssurveysstars: abundancesstars: generalMagellanic Cloudsgalaxies: photometryAstronomy & AstrophysicsThe Fourth S-PLUS Data Release: 12-filter photometry covering ∼3000 square degrees in the southern hemisphereArticulo de revista10.1051/0004-6361/202449725