activity
19972024
most citedDiscovery of the peculiar supernova 1998bw in the error box of GRB980425

1.9k citations · 4.8k across the 22 of their papers we have counts for

collaborators

22 papers

astro-ph.HE2024★ 1 cited

Nebular Nitrogen Line Emission in Stripped-Envelope Supernovae -- a New Progenitor Mass Diagnostic

Stan Barmentloo, Anders Jerkstrand, Koichi Iwamoto +4

Nitrogen is produced by CNO-cycling in massive stars, and can be ejected in significant amounts in supernova explosions. While in H-rich SNe, its [\ion{N}{II}] 6548, 6583 emission…

astro-ph.HE2016★ 35 cited

Impact of New Gamow-Teller Strengths on Explosive Type Ia Supernova Nucleosynthesis

Kanji Mori, Michael A. Famiano, Toshitaka Kajino +6

Recent experimental results have confirmed a possible reduction in the GT strengths of pf-shell nuclei. These proton-rich nuclei are of relevance in the deflagration and explos…

astro-ph.HE2013★ 12 cited

Gravitational Wave Memory from the Relativistic Jet of Gamma-Ray Bursts

Shota Akiba, Megumi Nakada, Chiyo Yamaguchi +1

The gravitational wave (GW) memory from a radiating and decelerating point mass is studied in detail. It is found that for isotropic photon emission the memory generated from the p…

astro-ph2008★ 30 cited

Observational Characteristics and Possible Asphericity of Over-Luminous Type Ia Supernovae

Keiichi Maeda, Koichi Iwamoto

A few Type Ia supernovae (SNe Ia) have been suggested to be an explosion of a super-Chandrasekhar-mass white dwarf (WD) to account for their large luminosities, requiring a large a…

astro-ph2003★ 58 cited

Hypernovae and Other Black-Hole-Forming Supernovae

K. Nomoto, K. Maeda, P. A. Mazzali +3

During the last few years, a number of exceptional core-collapse supernovae (SNe) have been discovered. Their kinetic energy of the explosions are larger by more than an order of m…

astro-ph2002★ 2 cited

The Type Ic Hypernova SN 2002ap

P. A. Mazzali, J. Deng, K. Maeda +31

Photometric and spectroscopic data of the energetic Type Ic supernova (SN) 2002ap are presented, and the properties of the SN are investigated through models of its spectral evolut…