HD 154672 b is a Hot Jupiter, as it is a closely orbiting planet with a high mass.
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N2K deliberately biased its search towards closely orbiting Jupiter-size planets (Hot Jupiters) in the orbit of metal-rich stars, as the consortium hoped to discover how the mass of a planet relates to its host star's metal content.
Using the radial velocity technique, the search for substellar companions has thus far failed to find a brown dwarf or extrasolar planet in the "hot zone" orbit around Kappa1 Ceti.
Hot Jupiters - a class of exoplanets like the one around Pegasi 51 (51 Pegasi b)
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