Figure 22 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 22.

Upper: SSFR as a function of galaxy local density in three stellar mass bins for our N3-selected supercluster member galaxies in A2255 and in the ANWS. The symbols are the same as in Figure 21. Lower: the fraction of each galaxy type as a function of local density.

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