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pro vyhledávání: '"Makarov, P. V."'
Autor:
Makarov, Valeri V., Cigan, Phil, Gordon, David, Johnson, Megan C., DiLullo, Christopher, Lambert, Sébastien
Published analyses of very long baseline interferometry (VLBI) data for the sources included in the third International Celestial Reference Frame (ICRF3) catalog have revealed object-specific, excess astrometric variability and quasi-coherent traject
Externí odkaz:
http://arxiv.org/abs/2411.16951
Autor:
Makarov, Valeri V.
Using the light curve time series data for more than 11.7 million variable sources published in the Gaia Data Release 3, the average magnitudes, colors, and variability parameters have been computed for 0.836 million Gaia CRF objects, which are mostl
Externí odkaz:
http://arxiv.org/abs/2408.17370
Astronomical time series often have non-uniform sampling in time, or irregular cadences, with long gaps separating clusters of observations. Some of these data sets are also explicitly non-Gaussian with respect to the expected model fit, or the simpl
Externí odkaz:
http://arxiv.org/abs/2405.12324
Autor:
Makarov, Valeri V., Tokovinin, Andrei
A large number of candidate binary stars with apparent acceleration on the sky has emerged from analysis of astrometric data collected by the Hipparcos, Tycho-2, and Gaia space missions. Although the apparent acceleration can serve as a relatively re
Externí odkaz:
http://arxiv.org/abs/2405.12315
Autor:
Makarov, Valeri V., Goldin, Alexey
Publikováno v:
Universe, 2024, 10, 15
(Abridged) Planets are surrounded by fractal surfaces (traditionally called Hill spheres), separating the inner zones of long-term stable orbital motion of their satellites from the outer space where the gravitational pull from the Sun takes over. Th
Externí odkaz:
http://arxiv.org/abs/2312.17049
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 527, Issue 3, January 2024, Pages 5131-5139
The gas giant Kepler-1658b has been inferred to be spiralling into its sub-giant F-type host star Kepler-1658a (KOI-4). The measured rate of change of its orbital period is $\dot{P}_{\rm orb}=-131^{+20}_{-22}\mathrm{ms/yr}$, which can be explained by
Externí odkaz:
http://arxiv.org/abs/2311.08801
Autor:
Makarov, Valeri V., Goldin, Alexey
Publikováno v:
Universe 2023, 9, 463
The transiting planet K2-18 b is one of the best candidates for a relatively nearby world harboring biological life. The long-term orbital evolution of this planet is investigated using theoretical and purely numerical techniques for two possible con
Externí odkaz:
http://arxiv.org/abs/2310.18754
Autor:
Anoshkin, Sergey S., Shishkin, Ivan I., Markina, Daria I., Logunov, Lev S., Demir, Hilmi Volkan, Rogach, Andrey L., Pushkarev, Anatoly P., Makarov, Sergey V.
Development of advanced optical data storage, information encryption, and security labeling technologies requires low-cost materials exhibiting local, pronounced, and diverse modification of their structure-dependent optical properties under external
Externí odkaz:
http://arxiv.org/abs/2309.06344
Autor:
Verkhogliadov, Grigorii, Haroldson, Ross, Gets, Dmitry, Zakhidov, Anvar A., Makarov, Sergey V.
Mixed halide perovskites undergo phase segregation, manifested as spectral red-shifting of photoluminescence spectra under illumination. In the iodine-bromide mixed perovskites, the origin of the low-energy luminescence is related to iodine-enriched
Externí odkaz:
http://arxiv.org/abs/2307.08392
The fundamental celestial reference frame (CRF) is based on two catalogs of astrometric positions, the third realization of the International Celestial Reference Frame (ICRF3), and the much larger Gaia~CRF, built from the third data release (DR3). Th
Externí odkaz:
http://arxiv.org/abs/2305.17755