Bun'ei Sato coauthored the discovery study of the transiting planet HD 149026 b. Combining a transit radius with a radial-velocity mass made its high bulk density informative about planetary interior models. The inference depends on both measured quantities and the assumed composition model.[ref]
The N2K Consortium. II. A Transiting Hot Saturn Around HD 149026 With a Large Dense Core by Bun'ei Sato and others. author list and the described study’s abstract or introductory account
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