The rapidly pulsating eclipsing binary NY Virginis has a period of 0.1 days. On a much longer timescale of 7.9 years, the system exhibits small amplitude cyclic variations which are associated with a third body in the system. A recent paper by Qian et. al. claims that this body is a giant circumbinary planet orbiting NY Vir at a distance of 3.3 astronomical units. There might be another planet in this system with an even longer orbital period, probably more than 15 years. 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.