Daisuke Toyouchi

Osaka University of Economics — Japan

Physics and Astronomy · Physical Sciences

8h-index217citations26works1.52yr avg
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Research Topics

Galaxies: Formation, Evolution, Phenomena(15), Astrophysical Phenomena and Observations(12), Astrophysics and Star Formation Studies(8), Astronomy and Astrophysical Research(8), Stellar, planetary, and galactic studies(7)

Publications26 total

Coherence of Supermassive Black Hole Binary Demographics with the nHz Stochastic Gravitational-wave Background
The Astrophysical Journal·2026Open Access
Clump-Scale Dust Attenuation in Epoch of Reionization Galaxies: Spatially Resolved Properties from FirstLight Simulations
arXiv (Cornell University)·2026Open Access
Clump-Scale Dust Attenuation in Epoch of Reionization Galaxies: Spatially Resolved Properties from FirstLight Simulations
ArXiv.org·2026Open Access
Forecasting Supermassive Black Hole Binary Gravitational Wave Probes: Prospects for Future Pulsar Timing Array and Space-Borne Detectors
arXiv (Cornell University)·2026Open Access
Forecasting Supermassive Black Hole Binary Gravitational Wave Probes: Prospects for Future Pulsar Timing Array and Space-Borne Detectors
ArXiv.org·2026Open Access
Cosmic Himalayas in CROCODILE : Probing the Extreme Quasar Overdensities by Count-in-Cells analysis and Nearest Neighbor Distribution
arXiv (Cornell University)·2025Open Access
Cosmic Himalayas in CROCODILE : Probing the Extreme Quasar Overdensities by Count-in-Cells analysis and Nearest Neighbor Distribution
ArXiv.org·2025Open Access
Bridging Theory and Observations: Insights into Star Formation Efficiency and Dust Attenuation in <i>z</i> &amp;gt; 5 Galaxies
Monthly Notices of the Royal Astronomical Society·2025· 3 citedOpen Access
Bridging Theory and Observations: Insights into Star Formation Efficiency and Dust Attenuation in $z &gt; 5$ Galaxies
arXiv (Cornell University)·2025Open Access
Radiation hydrodynamical simulations of super-Eddington mass transfer and black hole growth in close binaries
Monthly Notices of the Royal Astronomical Society·2024· 14 citedOpen Access
Radiation hydrodynamical simulations of super-Eddington mass transfer and black hole growth in close binaries
arXiv (Cornell University)·2024Open Access
The Assembly of Black Hole Mass and Luminosity Functions of High-redshift Quasars via Multiple Accretion Episodes
The Astrophysical Journal·2023· 22 citedOpen Access
Radiative feedback on supermassive star formation: the massive end of the Population III initial mass function
Monthly Notices of the Royal Astronomical Society·2022Open Access
The Assembly of Black Hole Mass and Luminosity Functions of High-redshift Quasars via Multiple Accretion Episodes
arXiv (Cornell University)·2022· 1 citedOpen Access
Top-heavy stellar mass distribution in galactic nuclei inferred from the universally high abundance ratio of [Fe/Mg]
Monthly Notices of the Royal Astronomical Society·2022Open Access
Rapid Growth of Seed Black Holes during Early Bulge Formation
The Astrophysical Journal·2022· 47 citedOpen Access
Top-heavy stellar mass distribution in galactic nuclei inferred from the\n universally high abundance ratio of [Fe/Mg]
arXiv (Cornell University)·2021· 21 citedOpen Access
Hunting wide-area optical surveys for high proper motion isolated neutron stars
Monthly Notices of the Royal Astronomical Society·2021· 3 cited
Hunting isolated neutron stars with proper motions from wide-area optical surveys
arXiv (Cornell University)·2021· 1 citedOpen Access
Gaseous dynamical friction under radiative feedback: do intermediate-mass black holes speed up or down?
Monthly Notices of the Royal Astronomical Society·2020· 32 citedOpen Access
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Frequent Co-authors

Kohei Inayoshi(8), R. Kuiper(6), Masashi Chiba(5), Kenta Hotokezaka(4), Kentaro Nagamine(4), Takashi Hosokawa(3), Masafusa Onoue(3), Wenxiu Li(3), K. Kusakabe(3), Yoshiyuki Inoue(3), Riouhei Nakatani(2), Kazuyuki Sugimura(2), Miho N. Ishigaki(2), Hidenobu Yajima(2), Andrea Ferrara(2), Masahiro Takada(2), Keitaro Takahashi(2), Yurina Nakazato(2), Kosei Matsumoto(2), Akio Inoue(2)