nuance: Efficient Detection of Planets Transiting Active Stars Article Swipe
L. J. Garcia
,
Daniel Foreman-Mackey
,
C. A. Murray
,
S. Aigrain
,
Dax L. Feliz
,
F. J. Pozuelos
·
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.3847/1538-3881/ad3cd6
YOU?
·
· 2024
· Open Access
·
· DOI: https://doi.org/10.3847/1538-3881/ad3cd6
The detection of planetary transits in the light curves of active stars, featuring correlated noise in the form of stellar variability, remains a challenge. Depending on the noise characteristics, we show that the traditional technique that consists of detrending a light curve before searching for transits alters their signal-to-noise ratio and hinders our capability to discover exoplanets transiting rapidly rotating active stars. We present nuance , an algorithm to search for transits in light curves while simultaneously accounting for the presence of correlated noise, such as stellar variability and instrumental signals. We assess the performance of nuance on simulated light curves as well as on the Transiting Exoplanet Survey Satellite light curves of 438 rapidly rotating M dwarfs. For each data set, we compare our method to five commonly used detrending techniques followed by a search with the Box-Least-Squares algorithm. Overall, we demonstrate that nuance is the most performant method in 93% of cases, leading to both the highest number of true positives and the lowest number of false-positive detections. Although simultaneously searching for transits while modeling correlated noise is expected to be computationally expensive, we make our algorithm tractable and available as the JAX -powered Python package nuance, allowing its use on distributed environments and GPU devices. Finally, we explore the prospects offered by the nuance formalism and its use to advance our knowledge of planetary systems around active stars, both using space-based surveys and sparse ground-based observations.
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- Type
- article
- Language
- en
- Landing Page
- https://doi.org/10.3847/1538-3881/ad3cd6
- https://iopscience.iop.org/article/10.3847/1538-3881/ad3cd6/pdf
- OA Status
- gold
- Cited By
- 3
- References
- 63
- Related Works
- 10
- OpenAlex ID
- https://openalex.org/W4398776101
All OpenAlex metadata
Raw OpenAlex JSON
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https://openalex.org/W4398776101Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.3847/1538-3881/ad3cd6Digital Object Identifier
- Title
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nuance: Efficient Detection of Planets Transiting Active StarsWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2024Year of publication
- Publication date
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2024-05-24Full publication date if available
- Authors
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L. J. Garcia, Daniel Foreman-Mackey, C. A. Murray, S. Aigrain, Dax L. Feliz, F. J. PozuelosList of authors in order
- Landing page
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https://doi.org/10.3847/1538-3881/ad3cd6Publisher landing page
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https://iopscience.iop.org/article/10.3847/1538-3881/ad3cd6/pdfDirect link to full text PDF
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YesWhether a free full text is available
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goldOpen access status per OpenAlex
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https://iopscience.iop.org/article/10.3847/1538-3881/ad3cd6/pdfDirect OA link when available
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Planet, Stars, Astrobiology, Exoplanet, Astronomy, PhysicsTop concepts (fields/topics) attached by OpenAlex
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3Total citation count in OpenAlex
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2025: 3Per-year citation counts (last 5 years)
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10Other works algorithmically related by OpenAlex
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