collaborators

10 papers

astro-ph.GA2026

Gaia parallax bias via spherical harmonics: A Python tool and discussion of possible causes

Valeri V. Makarov, Ciprian T. Berghea

Parallaxes in Gaia DR3 are known to suffer from a complex set of sky-correlated and magnitude-dependent offsets or biases at the level of a few tens of as. Estimated from a samp…

astro-ph.GA2026

Systematic Effects in Gaia CRF Photometry Related to Scanning Geometry and BP/RP excess factor

Valeri V. Makarov

I report a previously undocumented, large-amplitude systematic dependence of the median Gaia -band magnitude of CRF3 sources on \texttt{ra\_dec\_corr}, which reflects the prefer…

astro-ph.CO2026

Mapping the Universe as a Bianchi I cosmology with Gaia data

Valeri V. Makarov, Asta Heinesen, Thomas Schücker

Measurements of tangential drifts of distant quasars and galactic nuclei on the celestial sphere provide a novel and independent method of testing cosmological hypotheses. In this…

astro-ph.GA2026

The Peculiar Velocity of Messier~87 from Microarcsecond Geodetic VLBI Astrometry

Valeri V. Makarov, Phil Cigan, Kyle Corcoran

Our knowledge of the space velocity of Messier 87, which is the dominant galaxy in the Virgo cluster, has been limited to the radial velocity component. Using a cadence of precisio…

astro-ph.SR2025

Distributions of wide binary stars in theory and in Gaia data: III. Orbital momenta, masses, and manifestations of MOND

Valeri V. Makarov

Using the censored catalog of 103,169 resolved Gaia DR3 binary stars with accurate astrometric data for each component, a new observable, object-specific parameter is computed for…

astro-ph.EP2025

Initial conditions for tidal synchronisation of a planet by its moon

Valeri V. Makarov, Michael Efroimsky

Moons tidally interact with their host planets and stars. A close moon is quickly synchronised by the planet, or becomes captured in a higher spin-orbit resonance. However, the pla…