Keiichi Maeda

教授 / Professor

Kyoto University

Japan

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Professor Keiichi Maeda is a faculty member at Kyoto University, Japan. His research areas primarily include supernovae, focusing on their diversity, origins, and the surrounding environments of these explosive events. Recent publications highlight his investigations into Type Ia and Type II supernovae, as well as the dynamics of helium-rich detonation in white dwarfs.

Keiichi Maeda

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Articles (30)

Luminous, rapidly declining supernovae as stripped transitional objects in low-metallicity environments: The case of SN 2022lxg

Observational diversity of bright long-lived Type II supernovae

A Common Origin of Normal Type Ia Supernovae Suggested by the Photometric Diversity

SN 2023vbg: A Type IIn Supernova Resembling SN 2009ip, with a Long-duration Precursor and Early-time Bump

SN 2023xgo: Helium-rich Type Icn or Carbon-Flash Type Ibn supernova?

Diversity in Hydrogen-rich Envelope Mass of Type II Supernovae. III. The Mass-loss and Evolutionary Pathways of the Red Supergiant Progenitors

Inferring a Dense Confined Circumstellar Medium around Supernova Progenitors via Long-term Hydrodynamical Evolution

Discovery of young, oxygen-rich supernova remnants in PHANGS-MUSE galaxies

Cellular Dynamics of Helium-rich Detonation on Sub-Chandrasekhar Mass White Dwarf

Spectropolarimetry of a Nuclear Transient AT2023clx: Revealing the Geometrical Alignment between the Transient Outflow and the Nuclear Dusty Region

Intermediate-luminosity Type IIP SN 2021gmj: a low-energy explosion with signatures of circumstellar material

Dynamical properties of mildly relativistic ejecta produced by the mass-loading of gamma-ray burst jets in dense ambient media

The enigmatic double-peaked stripped-envelope SN 2023aew

Evidence for bipolar explosions in Type IIP supernovae

Three-dimensional Velocity Diagnostics to Constrain the Type Ia Origin of Tycho's Supernova Remnant

Viewing Explosion Models of Type Ia Supernovae through Insights from Terrestrial Cellular Detonation

STELLA Lightcurves of Energetic Pair-instability Supernovae in the Context of SN2018ibb

The aspherical explosions of the 03fg-like Type Ia supernovae 2021zny and 2022ilv revealed by polarimetry

Chandra’s Insights into SN 2023ixf

Light curve and spectral modelling of the type IIb SN 2020acat

Millimeter Observations of the Type II SN 2023ixf: Constraints on the Proximate Circumstellar Medium

Diagnosing the ejecta properties of engine-driven supernovae from observables in their initial phase

Photometry and spectroscopy of the Type Icn supernova 2021ckj

Resurrection of Type IIL Supernova 2018ivc: Implications for a Binary Evolution Sequence Connecting Hydrogen-rich and Hydrogen-poor Progenitors

Examining Neutrino–Matter Interactions in the Cassiopeia A Supernova

Systematic Investigation of Very-early-phase Spectra of Type Ia Supernovae

Inferring the Progenitor Mass–Kinetic Energy Relation of Stripped-envelope Core-collapse Supernovae from Nebular Spectroscopy

Light-curve modelling for the initial rising phase of rapidly evolving transients powered by continuous outflow

Initial flash and spectral formation of Type Ia supernovae with an envelope: applications to overluminous SNe Ia

SN 2020uem: a Possible Thermonuclear Explosion within a Dense Circumstellar Medium (II). The Properties of the CSM from Polarimetry and Light-curve Modeling

Collaborators (23)

Thomas Reynolds

Luca Izzo

Stuart Sim

Mark Gurwell

Koji Kawabata

Miika Pursiainen

Toshiki Sato

Tomonari Michiyama

Toshikazu Shigeyama

Takashi Yoshida

Kyle Medler

Kate Alexander

Shiu-Hang Lee

Akihiro Suzuki

Rubina Kotak

Seppo Mattila

Giorgos Leloudas

David Young

Ryou Ohsawa

Cosimo Inserra

Takaaki Tanaka

Miho Kawabata

Masatoshi Imanishi

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