Efficient modeling of correlated noise. III. Scalable methods for jointly modeling several observables' time series with Gaussian processes
J.-B. Delisle, N. Unger, N. C. Hara, D. S\'egransan

TL;DR
This paper introduces S+LEAF 2, a scalable Gaussian process framework that efficiently models multiple time series, such as stellar activity indicators and radial velocities, with linear computational cost, enabling analysis of large astronomical data sets.
Contribution
The paper presents S+LEAF 2, a novel Gaussian process method that scales linearly with data size for joint modeling of multiple observables, significantly reducing computational costs.
Findings
Successfully reanalyzed 246 radial velocity measurements with reduced computational cost
Achieved over two orders of magnitude decrease in processing time compared to previous methods
Demonstrated applicability to large astronomical data sets for exoplanet detection
Abstract
The radial velocity method is a very productive technique used to detect and confirm extrasolar planets. The most recent spectrographs, such as ESPRESSO or EXPRES, have the potential to detect Earth-like planets around Sun-like stars. However, stellar activity can induce radial velocity variations that dilute or even mimic the signature of a planet. A widely recognized method for disentangling these signals is to model the radial velocity time series, jointly with stellar activity indicators, using Gaussian processes and their derivatives. However, such modeling is prohibitive in terms of computational resources for large data sets, as the cost typically scales as the total number of measurements cubed. Here, we present S+LEAF 2, a Gaussian process framework that can be used to jointly model several time series, with a computational cost that scales linearly with the data set size.…
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