943 datasets found

Keywords: exoplanets

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  • The 10 parsec sample in the Gaia era

    A catalogue of 541 nearby (within 10pc of the sun) stars, brown dwarfs, and confirmed exoplanets in 336 systems, as well 21 candidates, compiled from SIMBAD and several other...
  • LIFE Target Database Cone Search

    The LIFE Target Star Database contains information useful for the planned LIFE mission_ (mid-ir, nulling interferometer in space). It characterizes possible target systems...
  • Coordinated microlensing survey observations with Kepler K2/C9 using VST

    The Kepler satellite has observed the Galactic center in a campaign lasting from April until the end of June 2016 (K2/C9). The main objective of the 99 hours for the...
  • The LIFE Target Star Database LIFETD

    The LIFE Target Star Database contains information useful for the planned LIFE mission_ (mid-ir, nulling interferometer in space). It characterizes possible target systems...
  • K2-157 light curves and RVs curves

    The formation and evolution of ultra-short-period (USP) rocky planets is poorly understood. However, it is widely thought that these planets could not have formed at their...
  • WASP-121b radial velocities from JWST NIRSpec

    We have conducted a planetary radial velocity measurement of the ultrahot Jupiter WASP-121b using JWST NIRSpec phase curve data. Our analysis reveals the Doppler shift of the...
  • Coronographic observations for M dwarfs companions

    We present Super-RDI, a unique framework for the application of reference star differential imaging (RDI) to Keck/NIRC2 high-contrast imaging observations with the vortex...
  • Non-transiting exoplanets

    Previous studies showed evidence of a dearth of close-in exoplanets around fast rotators, which can be explained by the combined action of intense tidal and magnetic...
  • Dark skies of the slightly eccentric WASP-18 b

    Ultra-hot Jupiters are gas giant exoplanets strongly irradiated by their star, which sets intense molecular dissociation leading to atmospheric chemistry dominated by ions and...
  • Phot. & RVs for 6 giant planets around cool dwarfs

    Transiting giant exoplanets around M-dwarf stars (GEMS) are rare, owing to the low-mass host stars. However, the all-sky coverage of TESS has enabled the detection of an...
  • HATS-38b & WASP-139b: LCs & RVs

    We constrain the sky-projected obliquities of two low-density hot Neptune planets, HATS-38 b and WASP-139 b, orbiting nearby G and K stars using Rossiter-McLaughlin (RM)...
  • TOI-2427 HARPS RVs and activity indicators

    Using high-precision photometry, NASA's TESS space mission has discovered many intriguing transiting planet candidates. These discoveries require ground-based follow-up...
  • Exoplanets and host stars Gaia spect. cat.

    Complete, accurate, and precise catalogues of exoplanet host star (EHS) properties are essential to derive high-quality exoplanet parameters, and, thus, to study individual...
  • TOI-762 and TIC 46432937: LCs data

    We present the discovery of TOI 762 A b and TIC 46432937 b, two giant planets transiting M-dwarf stars. Transits of both systems were first detected from observations by the...
  • TOI-771 RV datasets

    The origin and evolution of the sub-Neptune population is a highly debated topic in the exoplanet community. With the advent of JWST, atmospheric studies can now put...
  • 4 giant stars with planets radial velocities

    With around 200 detections of exoplanets around giant stars to date, our knowledge of the population of exoplanets orbiting evolved hosts more massive than the Sun remains...
  • SOPHIE data of Gliese 411

    Periodic radial velocity variations in the nearby M-dwarf star Gl 411 are reported, based on measurements with the SOPHIE spectrograph. Current data do not allow us to...
  • HD23472 radial velocity observations

    Comparing the properties of planets orbiting the same host star, and thus formed from the same accretion disc, helps in constraining theories of exoplanet formation and...
  • HD 75898 and HD 11506 radial velocities

    Due to observational biases, a large fraction of known exoplanets are short-period objects. However, the search for planets began more than 20 years ago, so it is already...
  • Multiplicity of stars with planets

    We intended to quantify the impact of stellar multiplicity on the presence and properties of exoplanets. We investigated all exoplanet host stars at less than 100 pc using the...
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