Figure 24 from AKARI Observation of the North Ecliptic Pole (NEP) Supercluster at z = 0.087: Mid-infrared View of Transition Galaxies

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AKARI Observation of the North Ecliptic Pole (NEP) Supercluster at z = 0.087: Mid-infrared View of Transition Galaxies

Authors: Jongwan Ko, Myungshin Im, Hyung Mok Lee, Myung Gyoon Lee, Seong Jin Kim, Hyunjin Shim, Yiseul Jeon, Ho Seong Hwang, Christopher N. A. Willmer, Matthew A. Malkan, Casey Papovich, Benjamin J. Weiner, Hideo Matsuhara, Shinki Oyabu, and Toshinobu Takagi

Ko et al. 2012 The Astrophysical Journal 745 181.

Provider: AAS Journals

Caption: Figure 24.

Spatial distribution of each galaxy type in Figure 23, on the smoothed galaxy number density maps for all supercluster member galaxies in A2255 (left) and in the ANWS (right). In the right panel, the three "+" signs indicate the center of X-ray detected groups with the mean redshifts given (Henry et al. 2006). North is up and east is to the left.

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