118 datasets found

Keywords: brown dwarfs

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  • 89 new utlra cool dwarfs comoving companions

    We report the identification of 89 new systems containing ultracool dwarf companions to main-sequence stars and white dwarfs, using the citizen science project Backyard Worlds:...
  • Polarization monitoring of 2MJ21392676+0220226

    Recent atmospheric models for brown dwarfs suggest that the existence of clouds in substellar objects is not needed to reproduce their spectra, nor their rotationally induced...
  • Tull RVels, rotation periods and Inclinations

    The orientation between a star's spin axis and a planet's orbital plane provides valuable information about the system's formation and dynamical history. For non-transiting...
  • KPIC radial velocity follow up of HR 7672 B

    The detection of satellites around extrasolar planets, so called exomoons, remains a largely unexplored territory. In this work, we study the potential of detecting these...
  • Light curve of microlensing MOA-2019-BLG-008L

    We report on the observations, analysis and interpretation of the microlensing event MOA-2019-BLG-008. The observed anomaly in the photometric light curve is best described...
  • NIR light curve of 2MASS J00501994-3322402

    Only a handful of late T brown dwarfs have been monitored for spectrophotometric variability, leaving incomplete the study of the atmospheric cloud structures of the coldest...
  • IR light curve of VHS1256-1257b in 2018 & 2020 epochs

    The photometric and spectral variability of brown dwarfs probes heterogeneous temperature and cloud distributions and traces the atmospheric circulation patterns. We present a...
  • RV measurements for 12 stars

    The observed scarcity of brown dwarfs in close orbits (within 10AU) around solar-type stars has posed significant questions about the origins of these substellar companions....
  • Southern extrasolar planets CORALIE survey. XIX

    A historical planet-search on a sample of 1647 nearby southern main sequence stars has been ongoing since 1998 with the CORALIE spectrograph at La Silla Observatory, with a...
  • 8 TOI RV curves and 2 TOI light curves

    The detection and characterization of exoplanets and brown dwarfs around massive AF-type stars is essential to investigate and constrain the impact of stellar mass on planet...
  • Lithium depletion boundary in stellar assoc.

    Stellar ages are key to improving our understanding of different astrophysical phenomena. However, many techniques to estimate stellar ages are highly model-dependent. The...
  • 54 massive companions detected with SOPHIE

    Brown-dwarfs (BD) are substellar objects with masses intermediate between planets and stars within about 13-80M_J_. While isolated brown-dwarfs are most likely produced by...
  • Spectra of brown dwarf candidates in the ONC

    I present an analysis of archival spectra of 200 sources toward the Orion Nebula Cluster (ONC) that were obtained with the Near-Infrared Spectrograph (NIRSpec) onboard the James...
  • New L subdwarfs, population properties

    We present 27 new L subdwarfs and classify five of them as esdL and 22 as sdL. Our L subdwarf candidates were selected with the UKIRT Infrared Deep Sky Survey and Sloan Digital...
  • NICMOS Kernel-phase Interferometry. I. Brown dwarfs

    Filling out the dearth of detections between direct imaging and radial velocity surveys will test theories of planet formation and (sub)stellar binarity across the full range of...
  • (Sub)Stellar companions of exoplanet hosts

    We present the latest results of an ongoing multiplicity survey of exoplanet hosts, which was initiated at the Astrophysical Institute and University Observatory Jena, using...
  • The Gaia ultracool dwarf sample

    We identify and investigate known late M, L, and T dwarfs in the Gaia second data release. This sample is being used as a training set in the Gaia data processing chain of the...
  • Log of SALT-RSS observations

    New spectra of 81 ultracool dwarfs (spectral types M7 and later) are discussed. Spectral classifications of 49 objects are available in the literature, while 32 objects are...
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