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Table · dataset · 2026

S-PLUS Fornax Project (S+FP)

Listed in IVOA Registry (Virtual Observatory)

Observational extragalactic catalogs over wide sky areas are essential for uncovering the large-scale structure of the Universe.

Description

They allow, among others, cosmological studies and density analyses that impose strong constraints on models of galaxy formation and evolution. By taking advantage of the wide field images and the 12 optical bands of the Southern Photometric Local Universe Survey (S-PLUS), we aim at providing a catalog of galaxies located, in projection, towards the Fornax galaxy cluster, within ~5 virial radii in right ascension (R.A.) and ~ 3virial radius in declination (Dec) around NGC 1399, the dominant galaxy of the cluster.

Such a catalog will allow unprecedented large-scale structure studies in that sky region. Supervised deep learning algorithms have been developed, utilizing neural networks complemented with dimensionality reduction techniques, to classify and separate spurious objects, stars and galaxies in a photometric catalog previously built for the S-PLUS Fornax Project (S+FP). That catalog was built using a combination of SExtractor configurations optimized for galaxy detection and characterization.

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A catalog of 119580 galaxies was obtained in the direction of the Fornax cluster containing photometric information in the 12 optical bands of S-PLUS complemented with GALEX (UV), VHS-VISTA (NIR) and AllWISE (MIR) data. We estimate photometric redshifts ({sigma}_NMAD_~0.0219) with a lower limit of zlim~0.03. Stellar masses, star formation rates (SFRs) and D4000N index estimates were obtained through a machine learning approach, by matching S-PLUS photometric data to SDSS spectroscopic data.

The completeness of the catalog (72%) was calculated by comparing with mock catalogs. Taking into account our zlim, we were able to identify 119230 background galaxies and to find 350 candidates to be Fornax members or infalling galaxies, not included in our compilation of 1005 galaxies previously reported in the literature. We were also able to classify the galaxies in our catalog as quiescent (43%), star-forming (39%) and transition (18%) galaxies.

In addition, 181 emission line galaxy (ELG) candidates were identified using the filter J0660. The spatial distribution of the galaxies in our catalog show projected overdensities that match 89 background clusters identified by eROSITA. This confirms the robustness of our catalog in tracing real structures.

In that context, we expect that the extragalactic catalog of the S+FP allows us to better understand the large-scale structure in the direction of the Fornax cluster, and to identify the substructures that are feeding Fornax.

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Stated by source
Infrared · Optical
Inferred from text
Image 65%
Provenance · 1 source records, 10 field assertions
SourceKeyLast seenRaw
IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/708/a20415 d agoJSON v1
FieldAssertionExtractorEvidence
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concepts[modality].ivoa_waveband:infraredsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].ivoa_waveband:opticalsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[modality].local:modality:imageenrichment · IVOA Registrykeyword-concept-rules@1.0.0title+description (65%)
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
titlesource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_title
updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0