gaspery: Optimized Scheduling of Radial Velocity Follow-Up Observations for Active Host Stars

TL;DR

Gaspery is an open-source tool that optimizes radial velocity follow-up observation schedules by accounting for stellar activity and correlated noise, improving exoplanet detection and characterization efficiency.

Contribution

It introduces a generalized Fisher Information framework incorporating stellar correlated noise, enabling optimized RV observation strategies tailored to stellar properties.

Findings

Optimized scheduling reduces RV uncertainty in noisy stellar environments.

Beat frequencies between orbital, stellar rotation, and observation epochs significantly impact information gain.

Gaspery effectively determines minimal observations needed for desired uncertainty levels.

Abstract

Radial velocity (RV) follow-up is a critical complement of transiting exoplanet surveys like the Transiting Exoplanet Survey Satellite (TESS ), both for validating discoveries of exoplanets and measuring their masses. Stellar activity introduces challenges to interpreting these measurements because the noise from the host star, which is often correlated in time, can result in high RV uncertainty. A robust understanding of stellar activity and how its timescales interact with the observing cadence can optimize limited RV resources. For this reason, in the era of over-subscribed, high-precision RV measurements, folding stellar activity timescales into the scheduling of observation campaigns is ideal. We present gaspery, an open-source code implementation to enable the optimization of RV observing strategies. Gaspery employs a generalized formulation of the Fisher Information for RV time series that also incorporates information about stellar correlated noise. We show that the information contained in an observing strategy can be significantly affected by beat frequencies between the orbital period of the planet, the stellar rotation period, and the observation epochs. We investigate how the follow-up observing strategy will affect the resulting radial velocity uncertainty, as a function of stellar properties such as the spot decay timescale and rotation period. We then describe two example use cases for gaspery: 1) calculating the minimum number of observations to reach an uncertainty tolerance in a correlated noise regime and 2) finding an optimal strategy given a fixed observing budget. Finally, we outline a prescription for selecting an observing strategy that is generalizable to different targets.