Analysis of radial velocity variations in multiple planetary systems
Andr\'as P\'al (1,2) ((1) Konkoly Observatory, (2) Department of, Astronomy, Lor\'and E\"otv\"os University)

TL;DR
This paper presents an algorithm for analyzing radial velocity data in multi-planet systems, accounting for planet-planet interactions to improve the accuracy of planetary parameter estimation.
Contribution
It introduces a novel algorithm for computing derivatives in radial velocity models that include planetary perturbations, enhancing analysis of complex systems.
Findings
Applied to systems HD 73526, HD 128311, and HD 155358.
Provides functions for spatial and barycentric coordinate calculations.
Facilitates joint analysis of transiting systems and high-precision astrometry.
Abstract
The study of multiple extrasolar planetary systems has the opportunity to obtain constraints for the planetary masses and orbital inclinations via the detection of mutual perturbations. The analysis of precise radial velocity measurements might reveal these planet-planet interactions and yields a more accurate view of such planetary systems. Like in the generic data modelling problems, a fit to radial velocity data series has a set of unknown parameters of which parametric derivatives have to be known by both the regression methods and the estimations for the uncertainties. In this paper an algorithm is described that aids the computation of such derivatives in case of when planetary perturbations are not neglected. The application of the algorithm is demonstrated on the planetary systems of HD 73526, HD 128311 and HD 155358. In addition to the functions related to radial velocity…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
