YARARA: Significant improvement of RV precision through post-processing of spectral time-series

TL;DR

YARARA is a post-processing pipeline that significantly improves radial-velocity measurement precision by cleaning spectral time-series from instrumental and atmospheric systematics, enabling better exoplanet detection.

Contribution

The paper introduces YARARA, a novel spectral cleaning pipeline that enhances RV precision by applying advanced corrections and PCA on spectral time-series, outperforming standard methods.

Findings

Achieved <1 m/s RV RMS over 13 years for HD10700, surpassing standard pipelines.

Reduced false signals and improved detection of known exoplanets.

Demonstrated that YARARA does not distort true Doppler signals.

Abstract

Aims: Even the most-precise radial-velocity instruments gather high-resolution spectra that present systematic errors that a data reduction pipeline cannot identify and correct for efficiently. In this paper, we aim at improving the radial-velocity precision of HARPS measurements by cleaning individual extracted spectra using the wealth of information contained in spectra time-series. Methods: We developed YARARA, a post-processing pipeline designed to clean high-resolution spectra from instrumental systematics and atmospheric contamination. Spectra are corrected for: tellurics, interference pattern, detector stitching, ghosts and fiber B contaminations as well as more advanced spectral line-by-line corrections. YARARA uses Principal Component Analysis on spectra time-series with prior information to disentangle contaminations from real Doppler shifts. We applied YARARA on three systems: HD10700, HD215152 and HD10180 and compared our results to the HARPS standard Data Reduction Software and the SERVAL post-processing pipeline. Results: On HD10700, we obtain radial-velocity measurements that present a rms smaller than 1 m/s over the 13 years of the HARPS observations, which is 20 and 10 % better than the HARPS Data Reduction Software and the SERVAL post-processing pipeline, respectively. We also injected simulated planets on the data of HD10700 and demonstrated that YARARA does not alter pure Doppler shifted signals. On HD215152, we demonstrated that the 1-year signal visible in the periodogram becomes marginal after processing with YARARA and that the signals of the known planets become more significant. Finally, on HD10180, the known six exoplanets are well recovered although different orbitals parameters and planetary masses are provided by the new reduced spectra.