Daniel Kasen

Lawrence Berkeley National Laboratory — United States

Physics and Astronomy · Physical Sciences

67h-index20.2kcitations339works7.62yr avg
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Research Topics

Gamma-ray bursts and supernovae(253), Pulsars and Gravitational Waves Research(123), Astrophysics and Cosmic Phenomena(71), Astrophysical Phenomena and Observations(69), Stellar, planetary, and galactic studies(60)

Publications334 total

Collapse of Magnetized White Dwarfs as site of Heavy Element Formation and Kilonova Signal
arXiv (Cornell University)·2026Open Access
Collapse of Magnetized White Dwarfs as site of Heavy Element Formation and Kilonova Signal
Zenodo (CERN European Organization for Nuclear Research)·2026Open Access
Collapse of Magnetized White Dwarfs as site of Heavy Element Formation and Kilonova Signal
ArXiv.org·2026Open Access
Collapse of Magnetized White Dwarfs as site of Heavy Element Formation and Kilonova Signal
Zenodo (CERN European Organization for Nuclear Research)·2026Open Access
Dynamics and Observational Signatures of Core-Collapse Supernovae with Central Engines: Hydrodynamics Simulations with Monte Carlo Post-Processing
Monthly Notices of the Royal Astronomical Society·2026Open Access
The Most Luminous Known Fast Blue Optical Transient AT 2024wpp: Unprecedented Evolution and Properties in the Ultraviolet to the Near-infrared
The Astrophysical Journal Letters·2026Open Access
The Emission and Suppression of Line Features in Luminous Transients
arXiv (Cornell University)·2026Open Access
The Emission and Suppression of Line Features in Luminous Transients
ArXiv.org·2026Open Access
ZTF25abjmnps (AT2025ulz) and S250818k: A Candidate Superkilonova from a Sub-threshold Sub-Solar Gravitational Wave Trigger
ArXiv.org·2025Open Access
The Most Luminous Known Fast Blue Optical Transient AT 2024wpp: Unprecedented Evolution and Properties in the X-Rays and Radio
The Astrophysical Journal Letters·2025· 2 citedOpen Access
Dynamics and Observational Signatures of Core-Collapse Supernovae with Central Engines: Hydrodynamics Simulations with Monte Carlo Post-Processing
arXiv (Cornell University)·2025· 1 citedOpen Access
An Integral-based Technique to Accelerate the Monte Carlo Radiative Transfer Computation for Supernovae
The Astrophysical Journal·2025Open Access
Simulated 3D $^{56}$Ni Distributions of Type IIp Supernovae
arXiv (Cornell University)·2025Open Access
2D end-to-end modelling of kilonovae from binary neutron star merger remnants
Monthly Notices of the Royal Astronomical Society·2025· 3 citedOpen Access
The Most Luminous Known Fast Blue Optical Transient AT 2024wpp: Unprecedented Evolution and Properties in the Ultraviolet to the Near-Infrared
arXiv (Cornell University)·2025Open Access
The Most Luminous Known Fast Blue Optical Transient AT 2024wpp: Unprecedented Evolution and Properties in the X-rays and Radio
arXiv (Cornell University)·2025Open Access
The Gravity Collective: A Comprehensive Analysis of the Electromagnetic Search for the Binary Neutron Star Merger GW190425
The Astrophysical Journal·2025· 2 citedOpen Access
SEDONA-GesaRaT: an AI-Accelerated Radiative Transfer Program for 3-D Supernova Simulations
arXiv (Cornell University)·2025Open Access
Neutrino heating in 1D, 2D, and 3D core-collapse supernovae: characterizing the explosion of high-compactness stars
Monthly Notices of the Royal Astronomical Society·2025· 6 citedOpen Access
Towards Exascale Astrophysics of Mergers and Supernovae (TEAMS)
2025
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Frequent Co-authors

Eliot Quataert(13), Brian D. Metzger(12), P. Nugent(11), A. Rest(10), R. J. Foley(8), D. A. Howell(8), M. R. Drout(7), E. Ramírez-Ruiz(6), Rodrigo Fernández(6), Jennifer Barnes(5), V. Ashley Villar(5), R. Chornock(5), R. Margutti(5), B. J. Shappee(5), Y. C. Pan(5), M. Sullivan(5), A. V. Filippenko(5), P. S. Cowperthwaite(4), E. Berger(4), M. Nicholl(4)