Hot Jupiter - Cold Jupiter: A complex sibling relation
Adriana Errico, Robert A. Wittenmyer, Jonathan Horner, Brad Carter, Valeria L\'opez

TL;DR
This study assesses the detectability of distant cold Jupiters in systems with Hot Jupiters using simulations of radial velocity data, revealing observational biases and guiding future survey strategies.
Contribution
It introduces a comprehensive simulation approach to evaluate the detectability of cold Jupiters around Hot Jupiter hosts, highlighting the importance of observational baseline over measurement precision.
Findings
Existing RV data are insensitive to Hot Jupiter-cold Jupiter pairs.
Longer observational baselines improve cold Jupiter detection.
Lower RV measurement precision does not significantly affect detection capability.
Abstract
A handful of planetary systems hosting a Hot Jupiter have been subsequently found to also host long-period giant planets. These ``cold Jupiters,'' giant planets residing beyond the snow line (3\,au), play an important role in the dynamical evolution of the system as a whole. In this work, we investigate the detectability of cold Jupiters around a sample of 28 well-studied Hot Jupiter host stars to estimate the occurrence rate of this distinctive system architecture. We perform extensive simulations using the combination of all publicly available radial velocity (RV) data for those stars with synthetic RV data. The synthetic data test observing strategies along three axes: cadence, duration, and measurement precision. For each scenario, we determine detection limits based on the semi-major axis at which a 1 Jupiter mass planet would be recovered 50\% of the time. We find the…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astro and Planetary Science · Scientific Research and Discoveries
