See [NASA ADS] for updated information. The metric of the publication is available here.
To summarize the list, the custom format of "%\g, \n"%\T", \n%\J, vol. %\V, %\p, (%\Y)\n" is useful.
Insights into non-axisymmetric instabilities in three-dimensional rotating supernova models with neutrino and gravitational-wave signatures, Takiwaki, Tomoya; Kotake, Kei; Foglizzo, Thierry Monthly Notices of the Royal Astronomical Society, Volume 508, Issue 1, pp.966-985, arXiv:2107.02933
Anisotropic emission of neutrino and gravitational-wave signals from rapidly rotating core-collapse supernovae, Takiwaki, Tomoya; Kotake, Kei Monthly Notices of the Royal Astronomical Society: Letters, Volume 475, Issue 1, p.L91-L95 arXiv:1711.01905
Three-dimensional simulations of rapidly rotating core-collapse supernovae: finding a neutrino-powered explosion aided by non-axisymmetric flows, Takiwaki, Tomoya; Kotake, Kei; Suwa, Yudai Monthly Notices of the Royal Astronomical Society: Letters, Volume 461, Issue 1, p.L112-L116 (2016); arXiv:1602.06759
A Comparison of Two- and Three-dimensional Neutrino-hydrodynamics Simulations of Core-collapse Supernovae, Takiwaki, Tomoya; Kotake, Kei; Suwa, Yudai The Astrophysical Journal, Volume 786, Issue 2, article id. 83, 8 pp. (2014); arXiv/1308.575
Three-dimensional Hydrodynamic Core-collapse Supernova Simulations for an 11 M_s Star with Spectral Neutrino Transport, Takiwaki, Tomoya; Kotake, Kei; Suwa, Yudai The Astrophysical Journal, Volume 749, Issue 2, article id. 98 (2012).; arXiv/1108.3989
Gravitational Wave Signatures of Magnetohydrodynamically Driven Core-collapse Supernova Explosions, Takiwaki, Tomoya; Kotake, Kei The Astrophysical Journal, Volume 743, Issue 1, article id. 30 (2011).; arXiv/1004.2896
Special Relativistic Simulations of Magnetically-dominated Jets from Collapsing Massive Stars, Tomoya Takiwaki, Kei Kotake,and Katsuhiko Sato The Astrophysical Journal, Volume 691, Issue 2, pp. 1360-1379 (2009).; arXiv/0712.1949
Magneto-driven Shock Waves in Core-Collapse Supernova, Tomoya Takiwaki, Kei Kotake, Shigehiro Nagataki and Katsuhiko Sato The Astrophysical Journal, Volume 616, Issue 2, pp. 1086-1094 (2004);_ astro-ph/0408388