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Optical and near-infrared observations of SN 2023ixf for over 600 days after the explosion
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Optical and near-infrared photometry of 94 type II supernovae from the Carnegie Supernova Project
J. P. Anderson, C. Contreras, M. D. Stritzinger, M. Hamuy, M. M. Phillips, N. B. Suntzeff, N. Morrell, S. González-Gaitán, C. P. Gutiérrez, C. R. Burns, E. Y. Hsiao, J. Anais, C. Ashall, C. Baltay, E. Baron, M. Bersten, L. Busta, S. Castellón, T. de Jaeger, D. DePoy, A. V. Filippenko, G. Folatelli, F. Förster, L. Galbany, C. Gall, et al. Astronomy & Astrophysics 692 A95 (2024) https://doi.org/10.1051/0004-6361/202244401
The progenitor of SN 2023ixf from hydrodynamical modeling
M. C. Bersten, M. Orellana, G. Folatelli, L. Martinez, M. P. Piccirilli, T. Regna, L. M. Román Aguilar and K. Ertini Astronomy & Astrophysics 681 L18 (2024) https://doi.org/10.1051/0004-6361/202348183
Intermediate-luminosity Type IIP SN 2021gmj: a low-energy explosion with signatures of circumstellar material
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Circumstellar interaction models for the early bolometric light curve of SN 2023ixf
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Interplay between neutrino kicks and hydrodynamic kicks of neutron stars and black holes
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Two-dimensional models of core-collapse supernova explosions assisted by heavy sterile neutrinos
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A Flat-spectrum Radio Transient at 122 Mpc Consistent with an Emerging Pulsar Wind Nebula
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Synthetic red supergiant explosion model grid for systematic characterization of Type II supernovae
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Simulated non-thermal emission of the supernova remnant G1.9 + 0.3
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Neutrino-driven massive stellar explosions in 3D fostered by magnetic fields via turbulent α-effect
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Light Curves of Type IIP Supernovae from Neutrino-driven Explosions of Red Supergiants Obtained by a Semianalytic Approach