Stellar mass and morphology in the cosmic web

In this work, we investigate if the location of galaxies within the large-scale structures (LSS) of the Universe leaves an imprint in their stellar mass (M*) and morphology. To this end, we attempt to disentangle the effects of local and large-scale environments in their distributions. We classify a sample of 25309 galaxies in the redshift range 0.02

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/710/A337
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/710/A337
Related Identifier https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/710/A337
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/710/A337
Provenance
Creator Torres-Rios G.; Verley S.; Perez I.; Argudo-Fernandez M.; Bidaran B.,Duarte Puertas S.; Gonzalez-Koda Y.K.
Publisher CDS
Publication Year 2026
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; Natural Sciences; Observational Astronomy; Physics