TOI-332: chains from the MCMC fit

<p>The 5 chains from the MCMC analysis of the TOI-332 system (paper in review). Chain files are 50,000 steps (rows), with no burn-in removed (1,000 steps are removed in our analysis).</p> <p>Parameters are given in the column headers, and described below:</p> <ul> <li>The lightcurve means (mean_tess28, mean_tess12, mean_lco1, mean_lco2, mean_lco3, mean_lco4, mean_lco5,&nbsp; mean_lco6)</li> <li>Intervals for the uniform priors (u_star_quadlimbdark____0, u_star_quadlimbdark____1, m_star_interval__ ,&nbsp; r_star_interval__, logr_interval__, b_impact__, period_interval__, t0_interval__, logK_interval__, offset_harps_interval__)</li> <li>And posterior values: <ul> <li>Log of the jitter on the HARPS data (where jitter is in m/s): log_jitter_harps&nbsp;&nbsp; &nbsp;</li> <li>The limb darkening: u_star__0, u_star__1&nbsp;&nbsp; &nbsp;</li> <li>Stellar mass (Msun): m_star</li> <li>Stellar radius (Rsun): r_star</li> <li>Log of the planet radius (where radius is in Rsun): logr&nbsp;&nbsp; &nbsp;</li> <li>Radius of the planet (Rsun): r_pl</li> <li>Planet-to-star radius ratio: ror</li> <li>Impact parameter: b</li> <li>Planet period (days): period</li> <li>Reference time of midtransit (BJD-2457000): t0</li> <li>Log of the RV semi-amplitude (where semi-amplitude is in m/s): logK</li> <li>Offset on the HARPS data (m/s): offset_harps</li> </ul> </li> </ul>