no code implementations • 24 Dec 2020 • Akihiro Suzuki, Matt Nicholl, Takashi J. Moriya, Tomoya Takiwaki
We suggest that the pulsational pair-instability SNe may provide a natural explanation for the massive CSM and the energetic explosion.
High Energy Astrophysical Phenomena
no code implementations • 23 Dec 2020 • Achille Fiore, Ting-Wan Chen, Anders Jerkstrand, Stefano Benetti, Riccardo Ciolfi, Cosimo Inserra, Enrico Cappellaro, Andrea Pastorello, Giorgos Leloudas, Steve Schulze, Marco Berton, Claudia Patricia Gutiérrez, Jamison Burke, Mariusz Gromadzki, Matt Nicholl, Arne Rau, Jesper Sollerman, Curtis McCully, Wen-fai Fong, Lluís Galbany, Daichi Hiramatsu, D. Andrew Howell, Erkki Kankare, Ragnhlid Lunnan, Tomás E. Müller-Bravo, David O Neill, David R. Young, Giacomo Terreran, Stefano Valenti
A CSM interaction scenario would imply a CSM mass of 5 Msun and an ejecta mass of 12 Msun.
High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
no code implementations • 3 Sep 2020 • Sebastian Gomez, Edo Berger, Peter K. Blanchard, Griffin Hosseinzadeh, Matt Nicholl, V. Ashley Villar, Yao Yin
This classifier can achieve a maximum purity of about 85\% (with 20\% completeness) when observing a selection of SLSN-I candidates.
High Energy Astrophysical Phenomena
