Figure 10 from VICS82: The VISTA–CFHT Stripe 82 Near-infrared Survey

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VICS82: The VISTA–CFHT Stripe 82 Near-infrared Survey

Authors: J. E. Geach, Y.-T. Lin, M. Makler, J.-P. Kneib, N. P. Ross, W.-H. Wang, B.-C. Hsieh, A. Leauthaud, K. Bundy, H. J. McCracken, J. Comparat, G. B. Caminha, P. Hudelot, L. Lin, L. Van Waerbeke, M. E. S. Pereira, and D. Mast

2017 The Astrophysical Journal Supplement Series 231 7.

Provider: AAS Journals

Caption: Figure 10.

iJK_s composite images of three distant clusters identified via the SZ effect with ACT (Hasselfield et al. 2013). Each panel is ﹩140^{\prime\prime} ﹩ on a side. VICS82 can clearly identify the passive galaxy population of each cluster, which allows us not only to assess the stellar mass content of rich distant clusters, but also to detect new clusters out to ﹩z\approx 1﹩ with masses that place them below the limit of SZ surveys.

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