Galaxy morphology in 5 medium redshift clusters

DOI

Following the study presented in our previous paper, based on the Nordic Optical Telescope (NOT) sample, which consists of five clusters of galaxies within the redshift range 0.18<=z<=0.25 imaged in the central 0.5-2Mpc in very good seeing conditions, we have studied the quantitative morphology of their bright galaxy population. We analyzed the surface brightness profiles of the galaxy population in those clusters, after performing simulations in order to check the reliability of the fits. We also derived a quantitative morphological classification.

Cone search capability for table J/A+A/506/1071/tablea1 (Results of the 2-dimensional surface brightness fit for the galaxies in the NOT sample)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35061071
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/506/1071
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/506/1071
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/506/1071
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/506/1071
Provenance
Creator Ascaso B.; Aguerri J.A.L.; Moles M.; Sanchez-Janssen R.; Bettoni D.
Publisher CDS
Publication Year 2010
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