Kai Ikuta

Project Assistant Professor

Hitotsubashi University

Japan

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About

Dr. Kai Ikuta is a Project Assistant Professor at Hitotsubashi University in Japan. His research focuses on stellar astrophysics, particularly the photometric and spectroscopic analysis of M-dwarf stars and their flares. His recent work includes studies on transiting exoplanets and the dynamics of stellar phenomena observed in various campaigns. He contributes to advancing our understanding of stellar behavior through multiwavelength observational techniques.

Articles (10)

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2025

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2025

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2025

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2025

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2024

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2024

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2024

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2024

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2024

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2024

Collaborators (7)

Vladimir Airapetian

Research Professor

American University

UNITED STATES

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Hiroyuki Maehara

助教/Assistant Professor

自然科学研究機構国立天文台/National Astronomical Observatory of Japan

JAPAN

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Akihiko Fukui

The Univeristy of Tokyo

JAPAN

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Julien Morin

University of Montpellier

FRANCE

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Aline Vidotto

Associate Professor

Leiden University

NETHERLANDS

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Kazunari Shibata

Kyoto University

JAPAN

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Takanori Kodama

Specially Appointed Associate Professor

JAPAN

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Kai Ikuta

Research Interests

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About

Articles (10)

Multiband, Multiepoch Photometry of the Spot-crossing System TOI-3884: Refined System Geometry and Spot Properties

The mass of TOI-654 b: A short-period sub-Neptune transiting a mid-M dwarf

Time evolution of a white-light flare accompanied by probable postflare loops on the M-type dwarf EV Lacertae

High-time-cadence Spectroscopy and Photometry of Stellar Flares on M-dwarf YZ Canis Minoris with Seimei Telescope and TESS. II. Statistical Properties of Blue/Red Asymmetries in the Hα Line

Simple Model for Temporal Variations of Hα Spectrum by an Eruptive Filament from a Superflare on a Solar-type Star

Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. II. Understanding Prominence Eruption through Data-driven Modeling and Observed Magnetic Environment

Sun-as-a-star Analysis of the X1.6 Flare on 2023 August 5: Dynamics of Postflare Loops in Spatially Integrated Observational Data

TOI-1199 b and TOI-1273 b: Two new transiting hot Saturns detected and characterized with SOPHIE and TESS

Characterization of starspots on a young M-dwarf K2-25: multi-band observations of stellar photometric variability and planetary transits

Apache Point Observatory (APO)/SMARTS Flare Star Campaign Observations. I. Blue Wing Asymmetries in Chromospheric Lines during Mid-M-Dwarf Flares from Simultaneous Spectroscopic and Photometric Observation Data

Collaborators (7)

Vladimir Airapetian

Hiroyuki Maehara

Akihiko Fukui

Julien Morin

Aline Vidotto

Kazunari Shibata

Takanori Kodama

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