Figure 1. The blue data points are from Swift/XRT observations, while the red line represents the best model to the data from

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Magnetar-powered Long Gamma-Ray Bursts and Connection to Superluminous Supernovae and Fast Radio Bursts

Authors: Yu-Qi Zhou, Shuang-Xi Yi, Yu-Peng Yang, Yan-Kun Qu, Ning Gai, Yanke Tang, Fa-Yin Wang

Yu-Qi Zhou et al 2026 The Astrophysical Journal Letters 1004 .

Provider: AAS Journals

Caption: Figure 1. The blue data points are from Swift/XRT observations, while the red line represents the best model to the data.

The complete figure set (139 images) is available in the online journal.

The X-ray light curves of 139 GRBs, excluding the 30 from F. Y. Wang et al. (2022a) (GRB 090205 may be a SGRB, P. D’Avanzo et al. 2010). The first 48 are GRBs with redshifts. The remaining 91 are GRBs with pseudo-redshifts.

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