1,037 datasets found

Keywords: exoplanets

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  • Mandel-Agol & dynamical parameters of KOI planets

    We use PyDynamicaLC, a model using the least number of--and the least correlated--degrees of freedom needed to derive a photodynamical model, to describe some of the...
  • Stellar and planetary param. of M-dwarf systems

    Planetary radii are derived for 218 exoplanets orbiting 161 M dwarf stars. Stellar radii are based on an analysis of APOGEE high-resolution near-IR spectra for a subsample of...
  • JWST transmission spectra of WASP-121b

    WASP-121 b has been established as a benchmark ultrahot Jupiter, serving as a laboratory for the atmospheric chemistry and dynamics of strongly irradiated extrasolar gas giants....
  • TOI-1243, TOI-4529, TOI-5388 RV datasets

    We report the confirmation of three transiting exoplanets orbiting TOI-1243 (LSPM J0902+7138), TOI-4529 (G 2-21) and TOI-5388 (Wolf 346) initially detected by TESS, through...
  • TOI-2431 RV and flux curves

    We present the discovery and confirmation of the ultra-short period (USP) planet TOI-2431 b orbiting a nearby (d~36pc) late K star (Teff=4109+/-28K) using observations from the...
  • TOI-3288 A b and TOI-4666 b light and RV curves

    Gas giant planets orbiting low-mass stars (Teff<=4600K) are uncommon outcomes of planet formation. Increasing the sample of well-characterised giants around early M dwarfs...
  • TOI-5789.01 planet candidate HARPS-N RVs

    Sub-Neptunes with planetary radii of R_p_=~2-4 R_{Earth} are the most common planets around solar-type stars in short-period (P<100d) orbits. It is still unclear, however,...
  • 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...
  • CARMENES DR1: Spectra

    The CARMENES instrument, installed at the 3.5 m telescope of the Calar Alto Observatory in Almería, Spain, was conceived to deliver high-accuracy radial velocity (RV)...
  • Carmenes DR1 Radial Velocity Time Series

    The CARMENES instrument, installed at the 3.5 m telescope of the Calar Alto Observatory in Almería, Spain, was conceived to deliver high-accuracy radial velocity (RV)...
  • 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...
  • Detection limits in the SHINE F150 survey

    In high-contrast imaging, a novel detection algorithm for angular differential imaging (ADI) sequences has recently been introduced: the Regime Switching Model (RSM). This...
  • Multiplanet system GJ 887

    GJ 877 is a bright M dwarf in the solar neighborhood with two currently reported nontransiting exoplanets with periods of 9d and 21d, along with an additional unconfirmed signal...
  • HD 128717 HARPS-N observations

    The transition regime between giant planets (GPs) and brown dwarfs (BDs) is still an open subject of study in exoplanetary science. A complete understanding of the population of...
  • 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...
  • RV data for Gliese 12

    Small temperate planets are prime targets for exoplanet studies due to their possible similarities with the rocky planets in the Solar System. M dwarfs are promising hosts since...
  • HARPS-N and CHEOPS data of HD 85426

    We provide a detailed characterisation of the planetary system orbiting HD 85426 (TOI-1774). This bright G-type star (M: 0.99M_{sun}_; R: 1.13R_{sun}; age: 7.4Gyr; Vmag: 8.25)...
  • Detectability of radio emission from exoplanets

    Like the magnetized planets in our Solar system, magnetized exoplanets should emit strongly at radio wavelengths. Radio emission directly traces the planetary magnetic fields...
  • Barium dwarfs with white dwarf companions

    We report three new barium (Ba) dwarfs lying in Sirius-like systems. They provide direct evidence that Ba dwarfs are companions to white dwarfs (WDs). Atmospheric parameters,...
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