Figure 1 from Measurement of the Rate Distribution of the Population of Repeating Fast Radio Bursts: Implications for Progenitor Models

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Measurement of the Rate Distribution of the Population of Repeating Fast Radio Bursts: Implications for Progenitor Models

Authors: C. W. James, S. Osłowski, C. Flynn, P. Kumar, K. Bannister, S. Bhandari, W. Farah, M. Kerr, D. R. Lorimer, J.-P. Macquart, C. Ng, C. Phillips, D. C. Price, H. Qiu, R. M. Shannon, and R. Spiewak

2020 The Astrophysical Journal Letters 895 L22.

Provider: AAS Journals

Caption: Figure 1.

Log-likelihood ﹩\mathrm{log}{ \mathcal L }﹩ as a function of fitting parameters ﹩{R}_{0}^{\min }﹩ and ζ, after being marginalized over ﹩{R}_{0}^{\max }﹩, for the standard parameter set γ = −0.9, k = 0.34, and α = −1.5. Confidence intervals of 68%, 90%, 95%, and 99.7% are shown by solid, dashed, dotted–dashed, and dotted lines, respectively.

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