Additional figures: Obliquities of exoplanet host stars. Nineteen new and updated measurements, and trends in the sample of 205 measurements

<p>Here we provide some additional figures as supporting material to Knudstrup et al. (2024).</p> <p><strong>Phase-folded light curves: </strong>The best-fitting models are shown as the white line in the top panel and the residuals are given in the bottom panel.</p> <p><strong>HD 118203 b:</strong> TESS 2 min. cadence data shown as gray points with error bars. Black markers are binned data in ~10 min. intervals.</p> <p><strong>HD 149193 b:</strong> TESS light curves 20 sec., 2 min., and 30 min. cadence data are shown in light gray, gray, and black, respectively.</p> <p><strong>K2-261 b:</strong> K2 light curve in black, TESS 20 sec. and 2 min. in light gray and gray, respectively. A light curve for each passband is shown.</p> <p><strong>K2-287 b:</strong> K2 30 min cadence shown in orange with CHEOPS 1 min. and ground-based 2 min. observations in light gray and gray, respectively. A light curve for each passband is also shown with a matching color.&nbsp;</p> <p><strong>KELT-3 b:</strong> TESS 2 min. cadence data shown in gray.</p> <p><strong>KELT-4Ab:</strong> TESS 2 min. cadence data shown in gray.</p> <p><strong>LTT 1445Ab:</strong> Black TESS 2 min. and gray TESS 20 sec.</p> <p><strong>TOI-451Ab:</strong> Unbinned 2 min. cadence data are shown in gray and in black the binned (~6 min.) data are shown.</p> <p><strong>TOI-813 b:</strong> TESS 20 sec., 2 min., and 30 min. cadence data are shown in light gray, gray, and black, respectively.</p> <p><strong>TOI-892 b:</strong> TESS 2 min. and 30 min. cadence data are shown in gray and black, respectively.</p> <p><strong>TOI-1130 c:</strong> TESS 20 sec. and 30 min. cadence data shown in gray and black, respectively.</p> <p><strong>WASP-50 b:</strong> TESS 20 sec. and 2 min. cadence data shown in gray and black, respectively.</p> <p><strong>WASP-59 b:</strong> TESS 2 min. cadence data shown in gray and ground-based 2 min. KeplerCam photometry in orange.</p> <p><strong>WASP-136 b:</strong> TESS 20 sec. and 2 min. cadence data shown in gray and black, respectively.</p> <p><strong>WASP-172 b:</strong> TESS 20 sec. and 30 min. cadence data shown in gray and black, respectively.</p> <p><strong>WASP-173Ab:</strong> TESS 20 sec. and 2 min. cadence data shown in gray and black, respectively.</p> <p><strong>WASP-186 b:</strong> TESS 20 sec., 2 min., and 30 min. cadence data are shown in light gray, gray, and black, respectively.</p> <p><strong>XO-7 b:</strong> TESS 20 sec., 2 min., and 30 min. cadence data are shown in light gray, gray, and black, respectively.</p> <p><strong>WASP-148 b:</strong> The MuSCAT-2 photometry obtained simultaneous with our spectroscopic transit observations. The observations in the different <em>griz</em> filters are shown as blue, orange, green, and red markers, respectively.</p> <p><strong>WASP-26 b:</strong> Unbinned 20 sec. cadence data from TESS are shown in gray and in black the binned (~6 min.) data are shown.</p> <div> <div> <div> <p>&nbsp;</p> <p><strong>Peak of the stacked CCFs:&nbsp;</strong>Similar to Fig. A.8. we show the peaks of the stacked CCFs for KELT-4 and XO-7 created by assuming the best-fitting value of b from the RV-RM fit.</p> <p><strong>KELT-4A:</strong> &nbsp;The gray contours show a peak around (v sin i⋆,&lambda;)=(6.0 km/s,90 deg). The red contours are the same as created from the posterior shown to the right in Fig. A.9.</p> <p><strong>XO-7: </strong>&nbsp;The gray contours show a peak around (v sin i⋆,&lambda;)=(4 km/s,-60 deg). The red contours are the same as created from the posterior shown to the right in Fig. A.28.</p> <p>&nbsp;</p> </div> </div> </div> <p><strong>References:</strong></p> <div> <div> <div> <p>Knudstrup, E., Albrecht, S. H., Winn, J. N., et al., 2024, arXiv:2408.09793</p> </div> </div> </div>