HAWK-I imaging of the X-ray luminous galaxy cluster XMMU J2235.3-2557 - The red sequence at z = 1.39
A&A, 489 3 (2008) 981-988
Published online: 2008-08-08
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PHYSICAL PROPERTIES OF FOUR SZE-SELECTED GALAXY CLUSTERS IN THE SOUTHERN COSMOLOGY SURVEY
Felipe Menanteau and John P. HughesThe Astrophysical Journal 694 (2) L136 (2009)
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SPECTROSCOPIC CONFIRMATION OF A MASSIVE RED-SEQUENCE-SELECTED GALAXY CLUSTER ATz= 1.34 IN THE SpARCS-SOUTH CLUSTER SURVEY
Gillian Wilson, Adam Muzzin, H. K. C. Yee, et al.The Astrophysical Journal 698 (2) 1943 (2009)
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Multi-wavelength study of XMMU J2235.3-2557: the most massive galaxy cluster at z > 1
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A comprehensive study of large-scale structures in the GOODS-SOUTH field up to ${\mathsf z} \sim $ 2.5
S. Salimbeni, M. Castellano, L. Pentericci, et al.Astronomy & Astrophysics 501 (3) 865 (2009)
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Large scale structures around radio galaxies atz~ 1.5
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Multiwavelength observations of a rich galaxy cluster at z $\thicksim$ 1
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The evolution of cluster early‐type galaxies over the past 8 Gyr
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AN INTENSIVEHUBBLE SPACE TELESCOPESURVEY FORz>1 TYPE Ia SUPERNOVAE BY TARGETING GALAXY CLUSTERS
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JKCS 041: a colour-detected galaxy cluster at $z_{\mathrm{phot}}$ ~ 1.9 with deep potential well as confirmed by X-ray data
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