Joint modelling of transit and stellar temperature using an MCMC ...
Joint modelling of transit and stellar temperature using an MCMC ...
Joint modelling of transit and stellar temperature using an MCMC ...
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CHAPTER 6. JOINT MODELLING OF TRANSIT AND STELLAR TEMPERATURE USING AN <strong>MCMC</strong> APPROACH 176<br />
Figure 6.3: The 2D <strong>MCMC</strong> chains with no prior on the T eff , <strong><strong>an</strong>d</strong> their posterior distributions.<br />
The chains are 1479000 steps long. Same colour line legend as Figure 6.2.<br />
Figure 6.4: The posterior distributions <strong>of</strong> a/R <strong><strong>an</strong>d</strong> i derived from the posterior distributions<br />
<strong>of</strong> k <strong><strong>an</strong>d</strong> b. The posterior distributions <strong>of</strong> T eff , M <strong><strong>an</strong>d</strong> R derived from k, are shown<br />
for comparison with Figure 6.7. Same colour line legend as Figure 6.2.
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