Line-by-line velocity measurements, an outlier-resistant method for precision velocimetry

We present a new algorithm for precision radial velocity (pRV) measurements, a line-by-line (LBL) approach designed to handle outlying spectral information in a simple but efficient manner. The effectiveness of the LBL method is demonstrated on two datasets, one obtained with SPIRou on Barnard'...

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Bibliographic Details
Published in:arXiv.org 2022-07
Main Authors: Artigau, Étienne, Cadieux, Charles, Cook, Neil J, Doyon, René, Vandal, Thomas, Donati, Jean-Françcois, Moutou, Claire, Delfosse, Xavier, Fouqué, Pascal, Eder Martioli, Bouchy, François, Parsons, Jasmine, Carmona, Andres, Dumusque, Xavier, Astudillo-Defru, Nicola, Bonfils, Xavier, Mignon, Lucille
Format: Article
Language:English
Subjects:
Algorithms
Cross correlation
Extrasolar planets
Outliers (statistics)
Radial velocity
Red dwarf stars
Template matching
Velocimetry
Online Access:Get full text
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Summary:We present a new algorithm for precision radial velocity (pRV) measurements, a line-by-line (LBL) approach designed to handle outlying spectral information in a simple but efficient manner. The effectiveness of the LBL method is demonstrated on two datasets, one obtained with SPIRou on Barnard's star, and the other with HARPS on Proxima Centauri. In the near-infrared, the LBL provides a framework for m/s-level accuracy in pRV measurements despite the challenges associated with telluric absorption and sky emission lines. We confirm with SPIRou measurements spanning 2.7 years that the candidate super-Earth on a 233-day orbit around Barnard's star is an artifact due to a combination of time-sampling and activity. The LBL analysis of the Proxima Centauri HARPS post-upgrade data alone easily recovers the Proxima b signal and also provides a 2-sigma detection of the recently confirmed 5-day Proxima d planet, but argues against the presence of the candidate Proxima c with a period of 1900 days. We provide evidence that the Proxima c signal is associated with small, unaccounted systematic effects affecting the HARPS-TERRA template matching RV extraction method for long-period signals. Finally, the LBL framework provides a very effective activity indicator, akin to the full width at half maximum derived from the cross-correlation function, from which we infer a rotation period of \(92.1^{+4.2}_{-3.5}\) days for Proxima.
ISSN:2331-8422
DOI:10.48550/arxiv.2207.13524