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A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). II. Physical Properties Derived from the SED Fitting with Optical, Infrared, and Radio Data

  • Authors: Yoshiki Toba, Takuji Yamashita, Tohru Nagao, Wei-Hao Wang, Yoshihiro Ueda, Kohei Ichikawa, Toshihiro Kawaguchi, Masayuki Akiyama, Bau-Ching Hsieh, Masaru Kajisawa, Chien-Hsiu Lee, Yoshiki Matsuoka, Akatoki Noboriguchi, Masafusa Onoue, Malte Schramm, Masayuki Tanaka, and Yutaka Komiyama

2019 The Astrophysical Journal Supplement Series 243 15.

  • Provider: AAS Journals

Caption: Figure 7.

(Top) WISE color–color diagram of 148 HSC–FIRST RGs with S/N > 3 in 3.4, 4.6, and 12 μm. Blue and red circles are SDSS- and HSC-level RGs, respectively. Yellow and green circles are SDSS-detected FIRST FR I and FR II RGs with r < 17.8 mag, respectively, that are obtained from Capetti et al. (2017a, 2017b). Regions with different color shading show typical MIR colors of different populations of objects (Wright et al. 2010). The solid lines illustrate the AGN selection wedge defined from Mateos et al. (2012, 2013). (Bottom) Histogram of rest-frame 1.4 GHz luminosity (L1.4 GHz) and rest-frame radio-loudness (Rrest) for objects inside (magenta) and outside (black) of the AGN wedge. The mean values are shown in dashed lines.

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