HD 28185 Revisited: An Outer Planet, Instead of a Brown Dwarf, On a Saturn-like Orbit
Alexander Venner, Qier An, Chelsea X. Huang, Timothy D. Brandt, Robert, A. Wittenmyer, Andrew Vanderburg

TL;DR
This study reanalyzes the HD 28185 system using 22 years of data, confirming the presence of a temperate giant planet and revising a second companion to a super-Jovian on a Saturn-like orbit, illustrating advances in exoplanet detection.
Contribution
The paper provides a comprehensive reanalysis of HD 28185, clarifying the nature of its planetary companions with updated parameters and demonstrating the routine detection of giant planets at large orbital distances.
Findings
HD 28185 b is a temperate giant planet with an Earth-like incident flux.
HD 28185 c is a super-Jovian planet with a Saturn-like orbit.
The study highlights the increasing routine detection of giant planets at ~10 AU.
Abstract
As exoplanet surveys reach ever-higher sensitivities and durations, planets analogous to the solar system giant planets are increasingly within reach. HD 28185 is a Sun-like star known to host a planet on an Earth-like orbit; more recently, a brown dwarf with a more distant orbit has been claimed. In this work we present a comprehensive reanalysis of the HD 28185 system, based on 22 years of radial velocity observations and precision Hipparcos-Gaia astrometry. We confirm the previous characterisation of HD 28185 b as a temperate giant planet, with its day orbital period giving it an Earth-like incident flux. In contrast, we substantially revise the parameters of HD 28185 c; with a new mass of we reclassify this companion as a super-jovian planet. HD 28185 c has an orbital period of years, a semi-major axis…
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