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The Bolometric Light-curve Modeling of 98 Type I Superluminous Supernovae Using the Magnetar- and the Circumstellar Interaction Models Reveals Surprisingly High Ejecta Masses
Multipeaked non-thermal light curves from magnetar-powered gamma-ray bursts
Conor M B Omand, Nikhil Sarin and Gavin P Lamb Monthly Notices of the Royal Astronomical Society 539(3) 1908 (2025) https://doi.org/10.1093/mnras/staf565
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1100 days in the life of the supernova 2018ibb
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The Type I superluminous supernova catalogue I: light-curve properties, models, and catalogue description
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Bumpy Superluminous Supernovae Powered by a Magnetar–Star Binary Engine
SN 2022jli: A Type Ic Supernova with Periodic Modulation of Its Light Curve and an Unusually Long Rise
T. Moore, S. J. Smartt, M. Nicholl, S. Srivastav, H. F. Stevance, D. B. Jess, S. D. T. Grant, M. D. Fulton, L. Rhodes, S. A. Sim, R. Hirai, P. Podsiadlowski, J. P. Anderson, C. Ashall, W. Bate, R. Fender, C. P. Gutiérrez, D. A. Howell, M. E. Huber, C. Inserra, G. Leloudas, L. A. G. Monard, T. E. Müller-Bravo, B. J. Shappee, K. W. Smith, et al. The Astrophysical Journal Letters 956(1) L31 (2023) https://doi.org/10.3847/2041-8213/acfc25
Detailed spectrophotometric analysis of the superluminous and fast evolving SN 2019neq
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Magnetar Flare-driven Bumpy Declining Light Curves in Hydrogen-poor Superluminous Supernovae