Figure 10 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 10.

Upper: histogram of the N3 absolute magnitude of galaxies in A2255 (left) and in the ANWS (right). The top axis shows stellar masses calculated from the linear relation in Figure 9. Vertical lines are our N3 magnitude cut. Lower: distribution of derived total IR luminosity L _IR (8–1000) for S11-detected galaxies in A2255 (left) and the ANWS (right). The top axis corresponds to SFR, using the Kennicutt (1998) relation.

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