A robust, template-free approach to precise radial velocity extraction
arXiv:1912.09563 · doi:10.1093/mnras/stz3599
Abstract
Doppler spectroscopy is a powerful tool for discovering and characterizing exoplanets. For decades, the standard approach to extracting radial velocities (RVs) has been to cross-correlate observed spectra with a weighted template mask. While still widely used, this approach is known to suffer numerous drawbacks, and so in recent years increasing attention has been paid to developing new and improved ways of extracting RVs. In this proof-of-concept paper we present a simple yet powerful approach to RV extraction. We use Gaussian processes to model and align all pairs of spectra with each other; without constructing a template, we combine pairwise RV shifts to produce accurate differential stellar RVs. Doing this on a highly-localized basis enables a data-driven approach to identifying and mitigating spectral contamination, even without the input of any prior astrophysical knowledge. We show that a crude implementation of this method applied to an inactive standard star yields RVs with comparable precision to and significantly lower rms variation than RVs from industry-standard pipelines. Though amenable to numerous improvements, even in its basic form presented here our method could facilitate the study of smaller planets around a wider variety of stars than has previously been possible.
27 pages, 16 figures. Accepted for publication in MNRAS
References in corpus (16)
- Spectrum radial velocity analyser (SERVAL). High-precision radial velocities and two alternative spectral indicators
- Stellar activity of planetary host star HD 189733
- Barycentric Corrections at 1 cm/s for precise Doppler velocities
- Cross-Correlation and Maximum Likelihood Analysis: A New Approach to Combine Cross-Correlation Functions
- A spectroscopy study of nearby late-type stars, possible members of stellar kinematic groups
- The HARPS search for southern extra-solar planets XXXV. Planetary systems and stellar activity of the M dwarfs GJ 3293, GJ 3341, and GJ 3543
- Disentangling Planets and Stellar Activity for Gliese 667C
- HARPS-N Solar Radial-Velocity Variations Are Dominated By Large, Bright Magnetic Regions
- Insights on the Spectral Signatures of Stellar Activity and Planets from PCA
- The N2K Consortium VI: Doppler Shifts Without Templates and Three New Short-Period Planets
- Impact of micro-telluric lines on precise radial velocities and its correction
- Pinning down the mass of Kepler-10c: the importance of sampling and model comparison
- HARPS3 for a Roboticized Isaac Newton Telescope
- Velocities from Cross-Correlation: A Guide for Self-Improvement
- TIRAVEL - Template Independent RAdial VELocity measurement
- Filtering out activity-related variations from radial velocities in a search for low-mass planets
Cited by in corpus (9)
- The EXPRES Stellar Signals Project II. State of the Field in Disentangling Photospheric Velocities
- Statistical methods for exoplanet detection with radial velocities
- A HARPS-N mass for the elusive Kepler-37d: a case study in disentangling stellar activity and planetary signals
- SOAP-GPU: Efficient Spectral Modelling of Stellar Activity Using Graphical Processing Units
- Applications of a Gaussian Process Framework for Modelling of High-Resolution Exoplanet Spectra
- Multi-Mask Least-Squares Deconvolution: Extracting RVs using tailored masks
- Spectral Line Depth Variability in Radial Velocity Spectra
- HiFLEx -- a highly flexible package to reduce cross-dispersed echelle spectra
- A Hermite-Gaussian Based Radial Velocity Estimation Method