= Bun'ei Sato
{c}
<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.<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]{ref}
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