Figure 2 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 2.

Spatial distribution (J2000.0) of 1943 HSC–FIRST radio galaxies (black points) in GAMA09H (top), WIDE12H (middle), and GAMA15H (bottom) field. Blue, green, and red squares represent survey footprint of KiDS, VIKING, and H-ATLAS, respectively. Those regions are completely covered by ALLWISE and TGSS. There are 754, 344, and 845 HSC–FIRST objects in the GAMA09H, WIDE12H, and GAMA15H, respectively.

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