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The Hipparcos-Gaia Catalog of Accelerations

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arxiv 1811.07283 v1 pith:SVCN2HDE submitted 2018-11-18 astro-ph.SR astro-ph.EPastro-ph.GAastro-ph.IM

The Hipparcos-Gaia Catalog of Accelerations

classification astro-ph.SR astro-ph.EPastro-ph.GAastro-ph.IM
keywords hipparcoscataloggaiaproperaccelerationsmeasurementsmotiondifferences
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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This paper presents a cross-calibrated catalog of Hipparcos and Gaia astrometry to enable their use in measuring changes in proper motion, i.e., accelerations in the plane of the sky. The final catalog adopts the reference frame of the second Gaia data release (DR2) and locally cross-calibrates both the scaled Hipparcos-Gaia DR2 positional differences and the Hipparcos proper motions themselves to this frame. This gives three nearly independent proper motion measurements per star, with the scaled positional difference usually being the most precise. We find that a linear combination of the two Hipparcos reductions is superior to either reduction on its own, and address error inflation for both Hipparcos and Gaia DR2. Our adopted error inflation is additive (in quadrature) for Hipparcos and multiplicative for Gaia. We provide the covariance matrices along with the central epochs of all measurements. Our final proper motion differences are accurately Gaussian with the appropriate variances, and are suitable for acceleration measurements and orbit fitting. The catalog is constructed with an eye toward completeness; it contains nearly 98\% of the Hipparcos stars. It also includes a handful of spurious entries and a few stars with poor Hipparcos reductions that the user must vet by hand. Statistical distributions of accelerations derived from this catalog should be interpreted with caution.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. A New Sirius-like System at Only 21 Parsecs: An Elusive White Dwarf Companion to the Nearby K-dwarf HD 38230

    astro-ph.SR 2026-07 conditional novelty 6.0

    HD 38230 B is a gravitationally bound white dwarf at 21 pc with a dynamical mass of 0.71 solar masses on a ~1400-year orbit.

  2. Gaia Exoplanet Orbits, Demographics, and Evolution Survey (GEODES): Characteristics of Three Long-Period Companions Accelerating their Host Stars

    astro-ph.EP 2026-05 conditional novelty 5.0

    Three accelerating stars yield one stellar companion at 166 AU, one 45 Jupiter-mass object at ~18 AU, and one 9.5 Jupiter-mass object at 6.4 AU that is 65% likely to be a planet.

  3. Gaia Exoplanet Orbits, Demographics, and Evolution Survey (GEODES): Characteristics of Three Long-Period Companions Accelerating their Host Stars

    astro-ph.EP 2026-05 conditional novelty 5.0

    GEODES characterizes three accelerating nearby stars, finding a stellar companion, a 45-Jupiter-mass brown dwarf at about 18 AU, and a 9.5-Jupiter-mass companion that is more likely a planet than a brown dwarf.