Figure 6 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 6.

(a) Rest-frame 1.4 GHz radio luminosity and (b) the absolute i-band magnitude at the rest frame as a function of redshift. Yellow and blue circles represent SDSS-detected RGs (Best & Heckman 2012) and RGs discovered by the VLA-COSMOS project (Smolčić et al. 2017a), respectively. Red circles represent HSC–FIRST RGs with reduced χ² ≤ 5.0.

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