The CARMENES search for exoplanets around M dwarfs. The impact of rotation and magnetic fields on the radial velocity jitter in cool stars
arXiv:2412.07691 · doi:10.1051/0004-6361/202450836
Abstract
Radial velocity (RV) jitter represents an intrinsic limitation on the precision of Doppler searches for exoplanets that can originate from both instrumental and astrophysical sources. We aim to determine the RV jitter floor in M dwarfs and investigate the stellar properties that lead to RV jitter induced by stellar activity. We determined the RV jitter in 239 M dwarfs from the CARMENES survey that are predominantly of mid to late spectral type and solar metallicity. We also investigated the correlation between stellar rotation and magnetic fields with RV jitter. The median jitter in the CARMENES sample is 3.1 m/s, and it is 2.3 m/s for stars with an upper limit of 2 km/s on their projected rotation velocities. We provide a relation between the stellar equatorial rotation velocity and RV jitter in M dwarfs based on a subsample of 129 well-characterized CARMENES stars. RV jitter induced by stellar rotation dominates for stars with equatorial rotation velocities greater than 1 km/s. A jitter floor of 2 m/s dominates in stars with equatorial rotation velocities below 1 km/s. This jitter floor likely contains contributions from stellar jitter, instrumental jitter, and undetected companions. We study the impact of the average magnetic field and the distributions of magnetic filling factors on the RV jitter. We find a series of stars with excess RV jitter and distinctive distributions of magnetic filling factors. These stars are characterized by a dominant magnetic field component between 2-4 kG. An RV jitter floor can be distinguished from RV jitter induced by activity and rotation based on the stellar equatorial rotation velocity. RV jitter induced by activity and rotation primarily depends on the equatorial rotation velocity. This RV jitter is also related to the distribution of magnetic filling factors, and this emphasizes the role of the magnetic field in the generation of RV jitter.
References in corpus (64)
- emcee: The MCMC Hammer
- Astrophysical magnetic fields and nonlinear dynamo theory
- The HARPS search for southern extra-solar planets XXXI. The M-dwarf sample
- ESPRESSO@VLT -- On-sky performance and first results
- Chromospheric Activity and Jitter Measurements for 2630 Stars on the California Planet Search
- Spectrum radial velocity analyser (SERVAL). High-precision radial velocities and two alternative spectral indicators
- A Gaussian process framework for modelling stellar activity signals in radial velocity data
- State of the Field: Extreme Precision Radial Velocities
- Radial Velocity Jitter in Stars from the California and Carnegie Planet Search at Keck Observatory
- CHIRON - A Fiber Fed Spectrometer for Precise Radial Velocities
- SOAP 2.0: A tool to estimate the photometric and radial velocity variations induced by stellar spots and plages
- The CARMENES search for exoplanets around M dwarfs: High-resolution optical and near-infrared spectroscopy of 324 survey stars
- Evidence for Magnetic Flux Saturation in Rapidly Rotating M Stars
- Detecting Planets Around Very Low Mass Stars with the Radial Velocity Method
- Search for exoplanets with the radial-velocity technique: quantitative diagnostics of stellar activity
- The CARMENES search for exoplanets around M dwarfs: Different roads to radii and masses of the target stars
- A catalogue of rotation and activity in early-M stars
- CARMENES input catalogue of M dwarfs. I. Low-resolution spectroscopy with CAFOS
- Rotation Velocities for M-dwarfs
- The low-level radial velocity variability in Barnard's star (=GJ 699). Secular acceleration, indications for convective redshift, and planet mass limits
- Magnetism, rotation, and nonthermal emission in cool stars -- Average magnetic field measurements in 292 M dwarfs
- The CARMENES search for exoplanets around M dwarfs. Two temperate Earth-mass planet candidates around Teegarden's Star
- SOAP. A tool for the fast computation of photometry and radial velocity induced by stellar spots
- Prime Focus Spectrograph (PFS) for the Subaru Telescope: Overview, recent progress, and future perspectives
- Magnetic fields of M dwarfs
- CARMENES input catalogue of M dwarfs: III. Rotation and activity from high-resolution spectroscopic observations
- A candidate short-period sub-Earth orbiting Proxima Centauri
- Planetary system around the nearby M dwarf GJ 357 including a transiting, hot, Earth-sized planet optimal for atmospheric characterization
- Accounting for velocity jitter in planet search surveys
- Correcting HIRES radial velocities for small systematic errors
- CARMENES input catalogue of M dwarfs IV. New rotation periods from photometric time series
- The CARMENES search for exoplanets around M dwarfs. Stellar atmospheric parameters of target stars with SteParSyn
- Numerical simulations of surface convection in a late M-dwarf
- Magnetic fields in M dwarfs from the CARMENES survey
- The CARMENES search for exoplanets around M dwarfs. Guaranteed time observations Data Release 1 (2016-2020)
- Characterisation of the radial velocity signal induced by rotation in late-type dwarfs
- The magnetic field and multiple planets of the young dwarf AU~Mic
- Modelling the photosphere of active stars for planet detection and characterization
- SPIRou Input Catalog: Activity, Rotation and Magnetic Field of Cool Dwarfs
- The CARMENES search for exoplanets around M dwarfs: Radial-velocity variations of active stars in visual-channel spectra
- Three-dimensional simulations of near-surface convection in main-sequence stars - II. Properties of granulation and spectral lines
- Unsigned magnetic flux as a proxy for radial-velocity variations in Sun-like stars
- The HADES RV Programme with HARPS-N@TNG II. Data treatment and simulations
- The CARMENES search for exoplanets around M dwarfs. Measuring precise radial velocities in the near infrared: the example of the super-Earth CD Cet b
- Astrophysical Insights into Radial Velocity Jitter from an Analysis of 600 Planet-search Stars
- The CARMENES search for exoplanets around M dwarfs -- LP 714-47b (TOI 442.01): Populating the Neptune desert
- Mid-to-Late M Dwarfs Lack Jupiter Analogs
- Convective blueshift strengths of 810 F to M solar-type stars
- The CARMENES search for exoplanets around M dwarfs: Convective shift and starspot constraints from chromatic radial velocities
- Constraining atmospheric parameters and surface magnetic fields with : an application to SPIRou spectra
- Stellar signal components seen in HARPS and HARPS-N solar radial velocities
- The CARMENES search for exoplanets around M dwarfs: Stable radial-velocity variations at the rotation period of AD~Leonis -- A test case study of current limitations to treating stellar activity
- The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc
- The CARMENES search for exoplanets around M dwarfs: Benchmarking the impact of activity in high-precision radial velocity measurements
- The IAG spectral atlas of the spatially resolved Sun: Centre-to-limb observations
- Spectral variability of photospheric radiation due to faculae II: Facular contrasts for cool main-sequence stars
- The CARMENES search for exoplanets around M dwarfs. Telluric absorption corrected high S/N optical and near-infrared template spectra of 382 M dwarf stars
- Rotational modulation of spectroscopic Zeeman signatures in low-mass stars
- The CARMENES search for exoplanets around M dwarfs. Diagnostic capabilities of strong K I lines for photosphere and chromosphere
- TOI-1801 b: A temperate mini-Neptune around a young M0.5 dwarf
- Unsigned magnetic flux proxy from solar optical intensity spectra
- TOI-4438 b: a transiting mini-Neptune amenable to atmospheric characterization
- Solar Photospheric Spectrum Microvariability I. Theoretical searches for proxies of radial-velocity jittering
- Properties of F Stars with Stable Radial Velocity Timeseries: A Useful Metric for Selecting Low-jitter F Stars
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