Direct Imaging Constraints on the Putative Exoplanet 14 Her c
Timothy J. Rodigas (1), Jared R. Males (1), Philip M. Hinz (1), Eric, E. Mamajek (2), Russell P. Knox (1) ((1) Steward Observatory, University of, Arizona, (2) University of Rochester Dept. of Physics & Astronomy)

TL;DR
This study uses deep direct imaging combined with RV data to constrain the properties of the potential exoplanet 14 Her c, narrowing down its possible mass, orbit, and eccentricity.
Contribution
It demonstrates how combining RV and direct imaging data can effectively constrain the parameters of a putative exoplanet.
Findings
Excluded companions >18 Mj beyond 25 AU at 5σ confidence
Constrained 14 Her c's mass to 3-42 Mj and semi-major axis to 7-25 AU
Highlighted the importance of RV/imaging overlap for exoplanet characterization
Abstract
We present results of deep direct imaging of the radial velocity (RV) planet-host star 14 Her (=GJ 614, HD 145675), obtained in the \lprime ~band with the Clio-2 camera and the MMT adaptive optics system. This star has one confirmed planet and an unconfirmed outer companion, suggested by residuals in the RV data. The orbital parameters of the unconfirmed object are not well constrained since many mass/semimajor axis configurations can fit the available data. The star has been directly imaged several times, but none of the campaigns has ruled out sub-stellar companions. With \about 2.5 hrs of integration, we rule out at 5 confidence 18 \mj ~companions beyond \about 25 AU, based on the \cite{baraffe} COND mass-luminosity models. Combining our detection limits with fits to the RV data and analytic dynamical analysis, we constrain the orbital parameters of 14 Her c to be:…
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