FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3103210132> ?p ?o ?g. }

• W3103210132 abstract "Context. 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. Aims. 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. Methods. 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 Teff, log g, and [Fe/H] show degeneracies, the surface gravity is determined independently using stellar evolutionary models. Results. 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(Teff) = 51 K, sigma(logg) = 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." @default.
• W3103210132 created "2020-11-23" @default.
• W3103210132 creator A5003134253 @default.
• W3103210132 creator A5008323018 @default.
• W3103210132 creator A5010685602 @default.
• W3103210132 creator A5024127683 @default.
• W3103210132 creator A5026962940 @default.
• W3103210132 creator A5027977555 @default.
• W3103210132 creator A5029519221 @default.
• W3103210132 creator A5043201067 @default.
• W3103210132 creator A5046535759 @default.
• W3103210132 creator A5047808099 @default.
• W3103210132 creator A5047871874 @default.
• W3103210132 creator A5052389738 @default.
• W3103210132 creator A5057314068 @default.
• W3103210132 creator A5057419286 @default.
• W3103210132 creator A5065044478 @default.
• W3103210132 creator A5074436179 @default.
• W3103210132 creator A5088454192 @default.
• W3103210132 date "2018-07-01" @default.
• W3103210132 modified "2023-10-12" @default.
• W3103210132 title "The CARMENES search for exoplanets around M dwarfs - Photospheric parameters of target stars from high-resolution spectroscopy" @default.
• W3103210132 cites W1531115531 @default.
• W3103210132 cites W1971519595 @default.
• W3103210132 cites W1975101526 @default.
• W3103210132 cites W1985663566 @default.
• W3103210132 cites W1993159000 @default.
• W3103210132 cites W2008908147 @default.
• W3103210132 cites W2019030320 @default.
• W3103210132 cites W2019132911 @default.
• W3103210132 cites W2032802648 @default.
• W3103210132 cites W2039579563 @default.
• W3103210132 cites W2049896064 @default.
• W3103210132 cites W2075195667 @default.
• W3103210132 cites W2092837737 @default.
• W3103210132 cites W2113074944 @default.
• W3103210132 cites W2117914263 @default.
• W3103210132 cites W2122728645 @default.
• W3103210132 cites W2133636837 @default.
• W3103210132 cites W2138613133 @default.
• W3103210132 cites W2157805129 @default.
• W3103210132 cites W2161459806 @default.
• W3103210132 cites W2513851308 @default.
• W3103210132 cites W2554366407 @default.
• W3103210132 cites W2565396336 @default.
• W3103210132 cites W2781271447 @default.
• W3103210132 cites W2899497983 @default.
• W3103210132 cites W2990014506 @default.
• W3103210132 cites W3098326557 @default.
• W3103210132 cites W3099997494 @default.
• W3103210132 cites W3101365627 @default.
• W3103210132 cites W3102212427 @default.
• W3103210132 cites W3102552291 @default.
• W3103210132 cites W3103531038 @default.
• W3103210132 cites W3103885327 @default.
• W3103210132 cites W3104158146 @default.
• W3103210132 cites W3105231016 @default.
• W3103210132 cites W3105716763 @default.
• W3103210132 hasPublicationYear "2018" @default.
• W3103210132 type Work @default.
• W3103210132 sameAs 3103210132 @default.
• W3103210132 citedByCount "23" @default.
• W3103210132 countsByYear W31032101322018 @default.
• W3103210132 countsByYear W31032101322019 @default.
• W3103210132 countsByYear W31032101322020 @default.
• W3103210132 countsByYear W31032101322021 @default.
• W3103210132 crossrefType "journal-article" @default.
• W3103210132 hasAuthorship W3103210132A5003134253 @default.
• W3103210132 hasAuthorship W3103210132A5008323018 @default.
• W3103210132 hasAuthorship W3103210132A5010685602 @default.
• W3103210132 hasAuthorship W3103210132A5024127683 @default.
• W3103210132 hasAuthorship W3103210132A5026962940 @default.
• W3103210132 hasAuthorship W3103210132A5027977555 @default.
• W3103210132 hasAuthorship W3103210132A5029519221 @default.
• W3103210132 hasAuthorship W3103210132A5043201067 @default.
• W3103210132 hasAuthorship W3103210132A5046535759 @default.
• W3103210132 hasAuthorship W3103210132A5047808099 @default.
• W3103210132 hasAuthorship W3103210132A5047871874 @default.
• W3103210132 hasAuthorship W3103210132A5052389738 @default.
• W3103210132 hasAuthorship W3103210132A5057314068 @default.
• W3103210132 hasAuthorship W3103210132A5057419286 @default.
• W3103210132 hasAuthorship W3103210132A5065044478 @default.
• W3103210132 hasAuthorship W3103210132A5074436179 @default.
• W3103210132 hasAuthorship W3103210132A5088454192 @default.
• W3103210132 hasConcept C100905312 @default.
• W3103210132 hasConcept C101638190 @default.
• W3103210132 hasConcept C121332964 @default.
• W3103210132 hasConcept C1276947 @default.
• W3103210132 hasConcept C13565188 @default.
• W3103210132 hasConcept C150846664 @default.
• W3103210132 hasConcept C151130387 @default.
• W3103210132 hasConcept C151730666 @default.
• W3103210132 hasConcept C163479331 @default.
• W3103210132 hasConcept C2779343474 @default.
• W3103210132 hasConcept C44870925 @default.
• W3103210132 hasConcept C4839761 @default.
• W3103210132 hasConcept C51244244 @default.
• W3103210132 hasConcept C86803240 @default.
• W3103210132 hasConcept C99465377 @default.
• W3103210132 hasConceptScore W3103210132C100905312 @default.

• next