Fig. 11

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1 and 2σ parameter posteriors for the lowest frequency and 12-month matching catalogue UCB that is eclipsing and localised to within 10 deg2 on the sky. The black diamonds on the 2D posteriors represent the LDC injected parameter values. One can see that the amplitude and inclination angle have not been recovered, and no correlation is visible in the A-ι plane. Increasing the number of MCMC steps and searching over a longer observation time are needed to better determine these parameters and recover the expected correlation between them.
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