Testing velocity kinks as a planet-detection method: Do velocity kinks in surface gas emission trace planetary spiral wakes in the midplane continuum?

<p>The contents of this repository supplements the publication:</p> <p>Speedie, J. & Dong, R. (2022). "Testing Velocity Kinks as a Planet Detection Method: Do Velocity Kinks in Surface Gas Emission Trace Planetary Spiral Wakes in the Midplane Continuum?", <em>Astrophysical Journal Letters</em>, 940(2), L43.</p> <p>Provided are six mp4 files. There is one for each of the following disks/planet candidates:</p> <ol> <li>HD 143006</li> <li>HD 163296 (Pinte et al. 2020 "#2" kink)</li> <li>HD 163296 (Izquierdo et al. 2022 "P94" kink)</li> <li>GW Lup</li> <li>Sz 129</li> <li>DoAr 25</li> </ol> <p>Each mp4 file contains 8 frames. Each frame is a figure like Figures 1-4 of Speedie & Dong (2022), where the continuum image has been re-imaged using the DSHARP calibrated measurement set with a different Briggs robust parameter: [-1, -0.5, -0.3, 0, 0.3, 0.5, 1, 2] and no uv-tapering.</p> <p>The calibrated measurements sets provided by the DSHARP Large Program were sourced from https://almascience.eso.org/almadata/lp/DSHARP/</p> <p>---------------------------------------------------------------------------------</p> <p>When you make use of material from this repository, please acknowledge:</p> <p>Speedie, J. & Dong, R. (2022). "Testing Velocity Kinks as a Planet Detection Method: Do Velocity Kinks in Surface Gas Emission Trace Planetary Spiral Wakes in the Midplane Continuum?", <em>Astrophysical Journal Letters</em>, 940(2), L43.</p>