Mass profile and dynamical status of the z ~ 0.8 galaxy cluster LCDCS 0504

Journal Article · Sun Jun 01 00:00:00 EDT 2014 · Astronomy and Astrophysics

DOI:https://doi.org/10.1051/0004-6361/201322447· OSTI ID:1289723

Guennou, L.; Biviano, A.; Adami, C.; Limousin, M.; Lima Neto, G. B.; Mamon, G. A.; Ulmer, M. P.; Gavazzi, R.; Cypriano, E. S.; Durret, F.; Clowe, D.; LeBrun, V.; Allam, S.; Basa, S.; Benoist, C.; Cappi, A.; Halliday, C.; Ilbert, O.; Johnston, D.; Jullo, E. ; Just, D.; Kubo, J. M.; Márquez, I.; Marshall, P.; Martinet, N.; Maurogordato, S.; Mazure, A.; Murphy, K. J.; Plana, H.; Rostagni, F.; Russeil, D.; Schirmer, M.; Schrabback, T.; Slezak, E.; Tucker, D.; Zaritsky, D.; Ziegler, B.

Context. Constraints on the mass distribution in high-redshift clusters of galaxies are currently not very strong.

• 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: 1289723
• Report Number(s): FERMILAB-PUB-14-244-AE-CD; arXiv:1403.3614; 1285935
• Journal Information: Astronomy and Astrophysics, Vol. 566; ISSN 0004-6361
• Publisher: EDP Sciences
• Country of Publication: United States
• Language: English

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79 ASTRONOMY AND ASTROPHYSICS