PTFO 8-8695 b is a Jupiter-sized candidate planet orbiting a T Tauri star. The orbit is rapidly precessing, causing it to stop transiting during part of its orbital evolution. According to Onitsuka et al. (2017), the observations are better explained by a circumstellar dust clump or the occultation of an accretion hotspot. Link to scientific paper Your name Note: Your commit will be vetted before it is merged into the public version. It is crucial that you include a link to a scientific publication. For more information on the meaning of the different datafields see the readme file in the Open Exoplanet Catalogue repository on github.