Figure 8 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

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation

Hi-Resolution Export to PDF PPT Format

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 8.

(a) The color excess (E(B − V)_*), (b) stellar mass, (c) SFR, (d) IR luminosity contributed from AGNs, (e) total IR luminosity, (f) radio spectral index (α_radio), and (g) q_IR of HSC–FIRST RGs as a function of redshift. The color code is i-band magnitude. The histograms show the SDSS-level (blue), HSC-level (red), and total (black) objects. The dashed lines are mean values of each quantity for SDSS-level (blue) and HSC-level (red) objects. 835 RGs are plotted in panels (a) to (e) while 190 RGs with FIRST and TGSS data are plotted in panels (f) and (g).

Other Images in This Article

Copyright and Terms & Conditions