Constraining binary neutron star population synthesis models using short gamma-ray burst data

Open Access

Fig. 4.

Same as Fig. 1 but assuming a universal top-hat jet with three different opening angles, θ_c = 5°, 10°, and 20°. These posteriors were obtained from the conditioned distribution P(f_j ∣ θ_c) (see Fig. 3). The model LK with α_CE = 0.5 does not have any samples below f_j ≤ 10 for θ_c = 5°.

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