The star system HD 38529 contains a yellow subgiant (the planet hosting star) and a red dwarf. The binary separation is 12000 astronomical units. A debris disc has been detected around the planet hosting star beyond 86 astronomical units. 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.