Extended Data Table 2 Best-fit parameters for our smoothly broken power-law fits to the radio light curves of GRB 221009A between 3 GHz and 17.69 GHz

From: Precise measurements of self-absorbed rising reverse shock emission from gamma-ray burst 221009A

  1. A smoothing parameter s = 2 is used. For further information on the fitting process see the Methods. The time of the light-curve peak and the flux density at the peak are given by tb and A, respectively. Fits are not made to the 10 and 1.5 GHz data due to lack of a clear peak and insufficient data, respectively.
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