activity
20062026
most citedTaking the Measure of the Universe: Precision Astrometry with SIM PlanetQuest

145 citations · 378 across the 23 of their papers we have counts for

collaborators

24 papers

astro-ph.GA2026

A posteriori correction of Gaia CRF proper motions using conditional probability and zero-parallax prior

Valeri V. Makarov

Precision of proper motions and positions given in the Gaia Celestial Reference Frame (CRF) catalog can be statistically improved introducing conditional probability based on the p…

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…