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SN 2018bsz: Significant Dust Formation in a Nearby Superluminous Supernova

  • Authors: T.-W. Chen, 婷琬 陳, S. J. Brennan, R. Wesson, M. Fraser, T. Schweyer, C. Inserra, S. Schulze, M. Nicholl, J. P. Anderson, E. Y. Hsiao, 亦麒 蕭, A. Jerkstrand, E. Kankare, E. C. Kool, T. Kravtsov, H. Kuncarayakti, G. Leloudas, C.-J. Li, 傳睿 李, M. Matsuura, M. Pursiainen, R. Roy, A. J. Ruiter, P. Schady, I. R. Seitenzahl, J. Sollerman, L. Tartaglia, L. Wang, R. M. Yates, S. Yang, 圣 杨, D. Baade, R. Carini, A. Gal-Yam, L. Galbany, S. González-Gaitán, M. Gromadzki, C. P. Gutiérrez, R. Kotak, K. Maguire, P. A. Mazzali, T. E. Müller-Bravo, E. Paraskeva, P. J. Pessi, G. Pignata, A. Rau, D. R. Young

T.-W. Chen et al 2026 The Astrophysical Journal 1009 .

  • Provider: AAS Journals

Caption: Figure 3.

SED fitting for SN 2018bsz at selected epochs. The luminosities were converted from the observed magnitudes after correcting for the Milky Way extinction (green circles) while empty triangles denote 3σ upper limits. The corresponding blackbody temperatures and radii are listed in Table 1.

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