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Title: Structure and substructure analysis of DAFT/FADA galaxy clusters in the [0.4–0.9] redshift range

Context. The DAFT/FADA survey is based on the study of ~90 rich(masses found in the literature >2 x 10^14 M_⊙)and moderately distant clusters (redshifts 0.4 < z < 0.9), all withHST imaging data available. This survey has two main objectives: to constrain dark energy(DE) using weak lensing tomography on galaxy clusters and to build a database (deepmulti-band imaging allowing photometric redshift estimates, spectroscopic data, X-raydata) of rich distant clusters to study their properties.
Authors:
;
Publication Date:
OSTI Identifier:
1331803
Report Number(s):
FERMILAB-PUB-13-678-A; arXiv:1311.6922
Journal ID: ISSN 0004-6361; 1266401
DOE Contract Number:
AC02-07CH11359
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astronomy and Astrophysics; Journal Volume: 561
Publisher:
EDP Sciences
Research Org:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Org:
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS