Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 429, Issue 1, Pages 833-848Publisher
OXFORD UNIV PRESS
DOI: 10.1093/mnras/sts379
Keywords
galaxies: clusters: individual: MACS J0358.8-2955
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Funding
- SAO [GO0-11140X, GO1-12172X]
- STScI [GO-12313]
- Marie Curie Career Integration grant [294074]
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We present results of a combined X-ray/optical analysis of the dynamics of the massive cluster MACS J0358.8-2955 (z = 0.428) based on observations with the Chandra X-ray Observatory, the Hubble Space Telescope and the Keck-I telescope on Mauna Kea. MACS J0358.8-2955 is found to be one of the most X-ray luminous clusters known at z > 0.3, featuring L-X,L-bol(
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