Figure 6 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 6.

Spectroscopic completeness as a function of the N3 apparent magnitude (top panel) and observed ( B − R) color and N3 apparent magnitude (bottom panel) of galaxies in the ANWS. Vertical dashed lines indicate the N3 magnitude cut used in this study.

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