Using Doppler Imaging To Model Stellar Activity And Search For Planets Around Sun-like Stars

Doppler Imaging (DI) is a well-established technique to map a physical field at a stellar surface from a time series of high-resolution spectra.

In this proof-of-concept study, we aim to show that traditional DI algorithms, originally designed for rapidly-rotating stars, have also the ability to model the activity of Sun-like stars, when observed with new-generation highly-stable spectrographs, and search for low-mass planets around them.

We used DI to retrieve the relative brightness distribution at the surface of the Sun from radial velocity (RV) observations collected by HARPS-N between 2022 and 2024. The brightness maps obtained with DI have a typical angular resolution of about 36 degrees and are a good match to low-resolution disc-resolved Dopplergrams of the Sun at epochs when the absolute, disc-integrated RV exceeds ~2 m/s. The RV residuals after DI correction exhibit a dispersion of about 0.6 m/s, comparable with existing state-of-the-art activity correction techniques.

Using planet injection-recovery tests, we also show that DI can be a powerful tool for blind planet searches, so long as the orbital period is larger than ~100days (i.e. 3 to 4 stellar rotation periods), and that it yields planetary mass estimates with an accuracy comparable to, for example, multi-dimensional Gaussian process regression. Finally, we highlight some limitations of traditional DI algorithms, which should be addressed to make DI a reliable alternative to state-of-the-art RV-based planet search techniques.

Baptiste Klein, Suzanne Aigrain, Michael Cretignier, Xavier Dumusque, Khaled Al Moulla, Jean-François Donati, Niamh K. O’Sullivan, Haochuan Yu, Andrew Collier Cameron, Oscar Barragán, Annelies Mortier, Alessandro Sozzetti

Comments: Accepted for publication in MNRAS
Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Instrumentation and Methods for Astrophysics (astro-ph.IM); Solar and Stellar Astrophysics (astro-ph.SR)
Cite as: arXiv:2508.12963 [astro-ph.EP] (or arXiv:2508.12963v1 [astro-ph.EP] for this version)
https://doi.org/10.48550/arXiv.2508.12963
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Related DOI:
https://doi.org/10.1093/mnras/staf1337
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Submission history
From: Baptiste Klein
[v1] Mon, 18 Aug 2025 14:37:26 UTC (1,586 KB)
https://arxiv.org/abs/2508.12963
Astrobiology