HD 99492 c was announced in 2010. Subsequent observations showed that the radial velocity variations attributed to this planet correlated with the stellar activity cycle, indicating that the planet is an artifact of the activity. 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.