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

Guennou, L.

doi:10.1051/0004-6361/201321208

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

Journal Article · Fri Jan 17 00:00:00 EST 2014 · Astronomy and Astrophysics

DOI:https://doi.org/10.1051/0004-6361/201321208· OSTI ID:1331803

Guennou, L.

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.

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Research Organization:: Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP)

DOE Contract Number:: AC02-07CH11359

OSTI ID:: 1331803

Report Number(s):: FERMILAB-PUB-13-678-A; arXiv:1311.6922; oai:inspirehep.net:1266401

Journal Information:: Astronomy and Astrophysics, Vol. 561; ISSN 0004-6361

Publisher:: EDP Sciences

Country of Publication:: United States

Language:: English

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

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