Tipo de publicación: Con árbitro

  • Publicación
    Confirmation of Color-dependent Centroid Shift Measured After 1.8 Years with HST
    We measured the precise masses of the host and planet in the OGLE-2003-BLG-235 system, when the lens and source were resolving, with 2018 Keck high resolution...
  • Publicación
    Confirmation of four hot Jupiters detected by TESS using follow-up spectroscopy from MaHPS at Wendelstein together with NEID and TRES
    We report the confirmation and characterization of four hot Jupiter-type exoplanets initially detected by TESS: TOI-1295 b, TOI-2580 b, TOI-6016 b, and TOI-6130...
  • Publicación
    Confirmation of the 12-year optical outburst cycle in blazar OJ 287.
    A large monitoring project, OJ-94, was set up with the aim of monitoring the blazar OJ 287 during the predicted optical outburst (in fall 1994, Sillanpaa et al...
  • Publicación
    Confirmation of the link between central star binarity and extreme abundance discrepancy factors in planetary nebulae
    It has recently been noted that there seems to be a strong correlation between planetary nebulae with close binary central stars and highly enhanced...
  • Publicación
    Confirmation of the planet hypothesis for the long-period radial velocity variations of β Geminorum
    Aims.Our aim is to confirm the nature of the long period radial velocity measurements for β Gem first found by Hatzes & Cochran (1993). Methods: .We present...
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    Confirmation of TiO absorption and tentative detection of MgH and CrH in the atmosphere of HAT-P-41b
    Understanding the role of optical absorbers is critical for linking the properties of the dayside and terminator atmospheres of hot Jupiters. This study aims to...
  • Publicación
    Confirming Herschel Candidate Protoclusters from ALMA/VLA CO Observations
    ALMA 870 μm continuum imaging has uncovered a population of blends of multiple dusty star-forming galaxies (DSFGs) in sources originally detected with the...
  • Publicación
    Confirming new white dwarf-ultracool dwarf binary candidates
    We present the results of a study to discover prospective new white dwarf-L dwarf binaries as identified by their near-infrared excesses in the UKIDSS catalogue...
  • Publicación
    Confirming the least massive members of the Pleiades star cluster
    We present optical photometry (i and Z band) and low-resolution spectroscopy (640-1015 nm) of very faint candidate members (J = 20.2-21.2 mag) of the Pleiades...