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Weak-Lensing Detection at z~1.3: Measurement of the Two Lynx Clusters with Advanced Camera for Surveys

M. J. Jee, R. L. White, H. C. Ford, G. D. Illingworth, J. P. Blakeslee, B. Holden, S. Mei

astro-pharXiv:astro-ph/0601334

Abstract

(Abridged) We present a HST/ACS weak-lensing study of RX J0849+4452 and RX J0848+4453, the two most distant (at z=1.26 and z=1.27, respectively) clusters yet measured with weak-lensing. The two clusters are separated by ~4' from each other and appear to form a supercluster in the Lynx field. Using our deep ACS F775W and F850LP imaging, we detected weak-lensing signals around both clusters at ~4 sigma levels. The mass distribution indicated by the reconstruction map is in good spatial agreement with the cluster galaxies. From the SIS fitting, we determined that RX J0849+4452 and RX J0848+4453 have similar projected masses of ~2.0x1014 solar mass and ~2.1x1014 solar mass, respectively, within a 0.5 Mpc (~60") aperture radius.

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