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Fast X-Ray Transients Produced by Off-axis Jet Cocoons from Long Gamma-Ray Bursts

  • Authors: Jian-He Zheng, Wenbin Lu

Jian-He Zheng and Wenbin Lu 2026 The Astrophysical Journal Letters 1003 .

  • Provider: AAS Journals

Caption: Figure A1.

Left panel: the energy distribution per logarithm of the terminal four-velocity. The blue line shows the Lc model at the fiducial resolution, while the orange line shows the same model at higher resolution. Both distributions are computed at tlab = 40 s when the jet head is reaching ∼10R. Right panel: EP WXT X-ray lightcurves. The solid lines are the fiducial lightcurves with ﹩{u}_{\infty ,{\rm{\max }}}=20﹩ in the Lc model that we show in the left panel of Figure 4. The dashed lines and dashed–dotted lines are lightcurves of the Lc models with ﹩{u}_{\infty ,{\rm{\max }}}=15﹩ and ﹩{u}_{\infty ,{\rm{\max }}}=30﹩, respectively. Colors indicate different viewing angles, as in the left panel of Figure 4.

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