Figure 4 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 4.

Histogram of redshift of HSC–FIRST RGs (solid line) and those with reduced χ² of the SED fitting smaller than 5.0 (shaded region). Red and blue line are the SDSS- and HSC-level objects in 1056 HSC–FIRST RGs. Red and blue regions are those in the 835 subsample (see Section 3.5).

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