Figure 5 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 5.

Examples of the SED (flux density as a function of wavelength in rest frame) and result of the SED fitting for our sample. The black points are photometric data where the down arrows mean 3σ upper limit. The blue, yellow, red, and green lines show stellar, AGN, SF, and radio component, respectively. The black solid lines represent the resultant SEDs. We provide best-fit SEDs for all 1056 HSC–FIRST RGs with derived physical properties (see Tables 3 and 4).

Other Images in This Article

Copyright and Terms & Conditions