Substructures in WINGS clusters (Ramella+, 2007)

Details Substructures in WINGS clusters (Ramella+, 2007) Substructures in WINGS clusters (Ramella+, 2007)

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ycat..34700039r&link_type=abstract

VizieR On-line Data Catalog: J/A+A/470/39. Originally published in: 2007A&A...470...39R

Computer Science

Clusters: Galaxy, Morphology

Scientific paper

WINGS is an all-sky, photometric (multi-band) and spectroscopic survey, whose global goal is the systematic study of the local cosmic variance of the cluster population and of the properties of cluster galaxies as a function of cluster properties and local environment.
The WINGS sample consists of 77 clusters selected from three X-ray flux limited samples compiled from ROSAT All-Sky Survey data, with constraints just on the redshift (0.04=20deg). The core of the project consists of wide-field optical imaging of the selected clusters in the B and V bands. The imaging data were collected using the WFC@INT (La Palma) and the WFI@MPG/ESO2.2 (La Silla) in the northern and southern hemispheres, respectively.
(1 data file).

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