Fig. 6
Flux intensity distribution of bursts detected from RRAT J1819−1458. The flux intensity distribution is generated by 266 detected bursts with SNR ≥ 6. The dashed curve line signifies that the intensity cumulative probability distribution is a power law. The power-law index α = 1.6 ± 0.2 is fitted from the numbers of bursts with intensities higher than 10.
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