Noriharu Watanabe, Norio Narita, Yasunori Hori. Nodal precession of a hot Jupiter transiting the edge of a late A-type star TOI-1518. Publications of the Astronomical Society of Japan. 2024. 76. 3. 374-385
Yasunori Hori, Akihiko Fukui, Teruyuki Hirano, Norio Narita, Jerome P. de Leon, Hiroyuki Tako Ishikawa, Joel D. Hartman, Giuseppe Morello, Nestor Abreu García, Leticia Álvarez Hernández, et al. The Discovery and Follow-up of Four Transiting Short-period Sub-Neptunes Orbiting M Dwarfs. The Astronomical Journal. 2024. 167. 6. 289-289
Masayuki Kuzuhara, Akihiko Fukui, John H. Livingston, José A. Caballero, Jerome P. de Leon, Teruyuki Hirano, Yui Kasagi, Felipe Murgas, Norio Narita, Masashi Omiya, et al. Gliese 12 b: A Temperate Earth-sized Planet at 12 pc Ideal for Atmospheric Transmission Spectroscopy. The Astrophysical Journal Letters. 2024. 967. 2. L21-L21
Kenji Kurosaki, Yasunori Hori, Masahiro Ogihara, Masanobu Kunitomo. Evolution of a Water-rich Atmosphere Formed by a Giant Impact on an Earth-sized Planet. The Astrophysical Journal. 2023. 957. 2. 67-67
Taiki Kagetani, Norio Narita, Tadahiro Kimura, Teruyuki Hirano, Masahiro Ikoma, Hiroyuki Tako ISHIKAWA, Steven Giacalone, Akihiko Fukui, Takanori Kodama, Rebecca Gore, et al. The mass of TOI-519 b: A close-in giant planet transiting a metal-rich mid-M dwarf. Publications of the Astronomical Society of Japan. 2023
Toshinori Shimizu, Taichi Uyama, Yasunori Hori, Motohide Tamura, Nicole Wallack. High-contrast Imaging around a 2 Myr-old CI Tau with a Close-in Gas Giant. 2022
Formation of Gas Giants with Small Cores; Core Accretion Model Revisited
(第6回太陽系外惑星大研究会 2010)
暴走ガス捕獲段階における原始ガス惑星のガス集積率
(日本天文学会 2009)
Gas Accretion Rate onto a Protoplanet during the Stage of Runaway Gas Accretion
(The 2nd Subaru International Conference:EXOPLANETS AND DISKS: THEIR FORMATION AND DIVERSITY 2009)
Gas Accretion Rates onto a Proto-Gas Giant Planet during the Runaway Gas Accretion Phase
(American Astronomical Society, DPS meeting #41 2009)
Incoming planetesimals captured in the envelope of a protoplanet during the formation stage; the total amount of heavy elements
(Symposium: Research Perspective of COE21, "How to Build Habitable Planets?" 2008)