A possible Trojan companion to Kepler-91b was identified by Placek et al. (2015). This companion was rejected based on unphysically high brightness temperatures inferred by the model, but Knuth et al. (2017) indicated that the analysis was not taking reflected light fully into account. 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.