The CARMENES search for exoplanets around M dwarfs - Photospheric parameters of target stars from high-resolution spectroscopy
arXiv:1802.02946 · doi:10.1051/0004-6361/201732312
Abstract
The new CARMENES instrument comprises two high-resolution and high-stability spectrographs that are used to search for habitable planets around M dwarfs in the visible and near-infrared regime via the Doppler technique. Characterising our target sample is important for constraining the physical properties of any planetary systems that are detected. The aim of this paper is to determine the fundamental stellar parameters of the CARMENES M-dwarf target sample from high-resolution spectra observed with CARMENES. We also include several M-dwarf spectra observed with other high-resolution spectrographs, that is CAFE, FEROS, and HRS, for completeness. We used a {chi}^2 method to derive the stellar parameters effective temperature T_eff, surface gravity log g, and metallicity [Fe/H] of the target stars by fitting the most recent version of the PHOENIX-ACES models to high-resolution spectroscopic data. These stellar atmosphere models incorporate a new equation of state to describe spectral features of low-temperature stellar atmospheres. Since T_eff, log g, and [Fe/H] show degeneracies, the surface gravity is determined independently using stellar evolutionary models. We derive the stellar parameters for a total of 300 stars. The fits achieve very good agreement between the PHOENIX models and observed spectra. We estimate that our method provides parameters with uncertainties of {sigma} T_eff = 51 K, {sigma} log g = 0.07, and {sigma} [Fe/H] = 0.16, and show that atmosphere models for low-mass stars have significantly improved in the last years. Our work also provides an independent test of the new PHOENIX-ACES models, and a comparison for other methods using low-resolution spectra. In particular, our effective temperatures agree well with literature values, while metallicities determined with our method exhibit a larger spread when compared to literature results.
References in corpus (32)
- The chemical composition of the Sun
- A grid of MARCS model atmospheres for late-type stars I. Methods and general properties
- A new extensive library of PHOENIX stellar atmospheres and synthetic spectra
- New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit
- A Non-Gray Theory of Extrasolar Giant Planets and Brown Dwarfs
- Models of Stars, Brown Dwarfs and Exoplanets
- How to Constrain Your M Dwarf: measuring effective temperature, bolometric luminosity, mass, and radius
- Stellar Diameters and Temperatures II. Main Sequence K & M Stars
- Theory of Low-Mass Stars and Substellar Objects
- Spectrum radial velocity analyser (SERVAL). High-precision radial velocities and two alternative spectral indicators
- Metallicity and Temperature Indicators in M dwarf K band Spectra: Testing New & Updated Calibrations With Observations of 133 Solar Neighborhood M dwarfs
- The H emission of nearby M dwarfs and its relation to stellar rotation
- Parallel Implementation of the PHOENIX Generalized Stellar Atmosphere Program
- The Effective Temperature Scale of M dwarfs
- The Solar Neighborhood XXXVII: The Mass-Luminosity Relation for Main Sequence M Dwarfs
- A catalogue of rotation and activity in early-M stars
- Prospecting in late-type dwarfs: a calibration of infrared and visible spectroscopic metallicities of late-K and M dwarfs spanning 1.5 dex
- CARMENES input catalogue of M dwarfs. I. Low-resolution spectroscopy with CAFOS
- Stellar Diameters and Temperatures V. Eleven Newly Characterized Exoplanet Host Stars
- CARMENES input catalogue of M dwarfs: III. Rotation and activity from high-resolution spectroscopic observations
- HATS-6b: A Warm Saturn Transiting an Early M Dwarf Star, and a Set of Empirical Relations for Characterizing K and M Dwarf Planet Hosts
- Atmospheres from very low-mass stars to extrasolar planets
- M Dwarf Metallicities and Giant Planet Occurrence: Ironing Out Uncertainties and Systematics
- CARMENES input catalogue of M dwarfs II. High-resolution imaging with FastCam
- Stellar parameters of early M dwarfs from ratios of spectral features at optical wavelengths
- Radial velocity signatures of Zeeman broadening
- Chemical Abundances of M-dwarfs from the APOGEE Survey. I. The Exoplanet Hosting Stars Kepler-138 and Kepler-186
- CAFE: Calar Alto Fiber-fed Echelle spectrograph
- A physically motivated and empirically calibrated method to measure effective temperature, metallicity, and Ti abundance of M dwarfs
- Fundamental M-dwarf parameters from high-resolution spectra using PHOENIX ACES models: I. Parameter accuracy and benchmark stars
- The physical mechanism behind M dwarf metallicity indicators and the role of C and O abundances
- Metallicity determination of M dwarfs - Expanded parameter range in metallicity and effective temperature
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- HADES RV Programme with HARPS-N at TNG XII. The abundance signature of M dwarf stars with planets
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- The CARMENES search for exoplanets around M dwarfs. Characterization of the nearby ultra-compact multiplanetary system YZ Ceti
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- A HARPS RV search for planets around young nearby stars
- The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc
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- Estimating fundamental parameters of nearby M dwarfs from SPIRou spectra
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- The CARMENES search for exoplanets around M dwarfs: Spectroscopic orbits of nine M-dwarf multiple systems, including two triples, two brown dwarf candidates, and one close M-dwarf-white dwarf binary
- The KOBE experiment: K-dwarfs Orbited By habitable Exoplanets. Project goals, target selection and stellar characterization
- The SOPHIE search for northern extrasolar planets XV. A Warm Neptune around the M-dwarf Gl378
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- Chemical Properties of the Local Disk and Halo. II. Abundances of 3745 M dwarfs and Subdwarfs from Improved Model Fitting of Low-Resolution Spectra
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- The CARMENES search for exoplanets around M dwarfs. Diagnostic capabilities of strong K I lines for photosphere and chromosphere
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- Estimating , radius and luminosity of M-dwarfs using high resolution optical and NIR spectral features
- Using autoencoders and deep transfer learning to determine the stellar parameters of 286 CARMENES M dwarfs
- A super-Earth on a close-in orbit around the M1V star GJ 740. A HADES and CARMENES collaboration
- Photometric Calibrations of M-dwarf Metallicity with Markov Chain Monte Carlo and Bayesian Inference
- Planetary companions orbiting the M dwarfs GJ 724 and GJ 3988. A CARMENES and IRD collaboration
- Ariel stellar characterisation II. Chemical abundances of carbon, nitrogen, and oxygen for 181 planet-host FGK dwarf stars
- The CARMENES search for exoplanets around M dwarfs. Behaviour of the Paschen lines during flares and quiescence
- Cool and Data-Driven: An Exploration of Optical Cool Dwarf Chemistry with Both Data-Driven and Physical Models
- GJ 357 b: A Super-Earth Orbiting an Extremely Inactive Host Star
- The CARMENES search for exoplanets around M dwarfs -- A deep transfer learning method to determine Teff and [M/H] of target stars
- Measurements of the Ca II infrared triplet emission lines of pre-main-sequence stars
- The CARMENES search for exoplanets around M dwarfs. A sub-Neptunian mass planet in the habitable zone of HN Lib
- Correlating Intrinsic Stellar Parameters with Mg II Self-Reversal Depths
- Performance of the Stellar Abundances and atmospheric Parameters Pipeline adapted for M dwarfs I. Atmospheric parameters from the spectroscopic module
- Rubidium abundances in solar metallicity stars
- Abundance analysis of benchmark M dwarfs
- M Subdwarf Research III. Spectroscopic Diagnostics for Breaking Parameter Degeneracy
- Calibrating the metallicity of M dwarfs in wide physical binaries with F-, G-, and K-primaries -- II: Carbon, oxygen, and odd-Z iron-peak abundances of the primary stars
- Exploring the stellar properties of M dwarfs with high-resolution spectroscopy from the optical to the near-infrared
- Discovery of a transiting hot water-world candidate orbiting Ross 176 with TESS and CARMENES
- Metallicities in M dwarfs: Investigating different determination techniques
- Refined M-type Star Catalog from LAMOST DR10: Measurements of Radial Velocities, , log , [M/H] and [/M]