Figure 2 from AKARI Observation of the North Ecliptic Pole (NEP) Supercluster at z = 0.087: Mid-infrared View of Transition Galaxies

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 2.

Second-order moments (from SExtractor) in the Maidanak R-band image vs. magnitude difference between MAG-AUTO and MAG-APER with 11'' diameter for N3 (left) and S11 (right). To determine aperture correction factors, we used the best fit (red dashed lines) for galaxies which are not contaminated by nearby objects. Black dashed and dotted lines show the mean value and the standard deviation of all sample galaxies in N3 (left) and S11 (right), respectively.

Other Images in This Article

Copyright and Terms & Conditions