Figure 9 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 9.

Stellar masses computed with BC03 vs. the N3 absolute magnitude of galaxies in the ANWS. Here we used 102 galaxies for which five or more bands were used in the SED fits. The solid line indicates the best fit (log M _*/ M _☉ = –0.524 × M _N3 – 0.810), and the two dashed lines represent the standard deviation of residuals to this fit (σ = 0.255).

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