690 datasets found

Keywords: stellar distance

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  • Bp-Ap stars HR-diagram from Hipparcos data

    Using Hipparcos (Cat. ) parallaxes and proper motions together with radial velocity data, the luminosity calibration and kinematics of Bp-Ap stars have been obtained. The used...
  • Mass segregation in open clusters

    On the basis of the best available member list and duplicity information, we have studied the radial structure of Praesepe and of the very young open cluster NGC 6231. We have...
  • Metal-poor stars spectroscopy. II

    Models of post-main sequence stellar evolution of VandenBerg & Bell have been applied to determine spectroscopic masses and distances for metal-poor stars. Careful...
  • Cartesian catalog of 30 million Gaia sources

    Accurate measurements of stellar positions and velocities are crucial for studying galactic and stellar dynamics. We aim to create a Cartesian catalog from Gaia DR3 to serve as...
  • StarHorse2, Gaia EDR3 photo-astrometric distances

    We present a catalogue of 362 million stellar parameters, distances, and extinctions derived from Gaia's Early Data Release (EDR3) cross-matched with the photometric catalogues...
  • Distances to 1.47 billion stars in Gaia EDR3

    Stellar distances constitute a foundational pillar of astrophysics. The publication of 1.47 billion stellar parallaxes from Gaia is a major contribution to this. Yet despite...
  • StarHorse, Gaia DR2 photo-astrometric distances

    Combining the precise parallaxes and optical photometry delivered by Gaia's second data release with the photometric catalogues of Pan-STARRS1, 2MASS, and AllWISE, we derived...
  • Distances to 1.33 billion stars in Gaia DR2

    For the majority of stars in the second Gaia data release, reliable distances cannot be obtained by inverting the parallax. A correct inference procedure must instead be used to...
  • A comprehensive analysis of Spitzer supernovae

    The mid-infrared (mid-IR) wavelength regime offers several advantages for following the late-time evolution of supernovae (SNe). First, the peaks of the SN spectral energy...
  • Simulated exoplanets from TESS list of targets

    The Transiting Exoplanet Survey Satellite (TESS) has a goal of detecting small planets orbiting stars bright enough for mass determination via ground-based radial velocity...
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