Extended Data Fig. 2: Power-law fits to our multi-frequency radio observations of GRB 221009A. | Nature Astronomy

Extended Data Fig. 2: Power-law fits to our multi-frequency radio observations of GRB 221009A.

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

Extended Data Fig. 2: Power-law fits to our multi-frequency radio observations of GRB 221009A.

A broken power-law fit to each radio band where we observe a clear peak. The results of the fits are giving in Extended Data Table 2. The rise and decay power law indices follow Frise ∝ t1.34±0.02 and Fdecay ∝ t−0.82±0.04, respectively. Error bars represent 1σ uncertainties.

Back to article page