Figure 10 from 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

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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 10.

Color–color diagram of r − i and i − z. The 1943 HSC–FIRST RG sample, and 835 RGs whose physical properties are studied in this work, are shown in black and magenta circles, respectively. Histogram of each color is also shown with solid lines (an entire sample of 1943 objects) and magenta-shaded regions (a subsample of 835 objects).

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