The distribution and physical properties of high-redshift [OIII] emitters in a cosmological hydrodynamics simulation

MLA

Moriwaki, Kana, et al. The Distribution and Physical Properties of High-Redshift [OIII] Emitters in a Cosmological Hydrodynamics Simulation. 2018. EBSCOhost, https://doi.org/10.1093/mnrasl/sly167.

APA

Moriwaki, K., Yoshida, N., Shimizu, I., Harikane, Y., Matsuda, Y., Matsuo, H., Hashimoto, T., Inoue, A. K., Tamura, Y., & Nagao, T. (2018). The distribution and physical properties of high-redshift [OIII] emitters in a cosmological hydrodynamics simulation. https://doi.org/10.1093/mnrasl/sly167

Chicago

Moriwaki, Kana, Naoki Yoshida, Ikkoh Shimizu, Yuichi Harikane, Yuichi Matsuda, Hiroshi Matsuo, Takuya Hashimoto, Akio K. Inoue, Yoichi Tamura, and Tohru Nagao. 2018. “The Distribution and Physical Properties of High-Redshift [OIII] Emitters in a Cosmological Hydrodynamics Simulation.” doi:10.1093/mnrasl/sly167.