The chart shows the distribution of publications by all Research.com ranked scientists in the field of Physics in 2026. The highlighted bar marks where Yuri Y. Kovalev sits on this spectrum.
This scientist: 438 publications — 45th percentile
45% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 1,469 publications or more.
The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where Yuri Y. Kovalev sits on this spectrum.
This scientist: 90 D-Index — 40th percentile
40% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
Yuri Y. Kovalev is affiliated with the Moscow Institute of Physics and Technology in the Russian Federation. Their research primarily focuses on the field of Physics and Astronomy, with a strong emphasis on subfields such as Astronomy and Astrophysics, Nuclear and High Energy Physics, and related interdisciplinary areas including Atomic and Molecular Physics, and Optics, as well as Electrical and Electronic Engineering.
Their work spans various main research topics, notably including Astrophysics and Cosmic Phenomena, Radio Astronomy Observations and Technology, Gamma-ray Bursts and Supernovae, Neutrino Physics Research, Astrophysical Phenomena and Observations, Galaxies: Formation, Evolution, Phenomena, and aspects of Dark Matter and Cosmic Phenomena.
Kovalev has contributed to several academic papers published in reputable venues. Notable publications include:
Kovalev's research outputs frequently appear in venues such as arXiv (Cornell University), Monthly Notices of the Royal Astronomical Society, Astronomy and Astrophysics, The Astrophysical Journal, and Galaxies.
Their collaborative work includes multiple joint publications with frequent co-authors:
The focus of Kovalev's studies involves detailed investigations into phenomena surrounding active galactic nuclei (AGN), high-energy neutrinos, jet structures in galaxies, and observations derived from very long baseline array (VLBA) experiments. Their research contributes to the understanding of astrophysical processes and the technological methods used for radio astronomy observations.
A. A. Abdo;A. A. Abdo;M. Ackermann;I. Agudo;M. Ajello
M. L. Lister;M. F. Aller;H. D. Aller;D. C. Homan
M. L. Lister;M. F. Aller;H. D. Aller;D. C. Homan
M. L. Lister;H. D. Aller;M. F. Aller;M. H. Cohen
M. L. Lister;M. H. Cohen;D. C. Homan;M. Kadler
K. I. Kellermann;M. L. Lister;M. L. Lister;D. C. Homan;D. C. Homan;R. C. Vermeulen
M. L. Lister;H. D. Aller;M. F. Aller;M. H. Cohen
Y. Y. Kovalev;Y. Y. Kovalev;K. I. Kellermann;M. L. Lister;D. C. Homan
A. A. Abdo;A. A. Abdo;M. Ackermann;M. Ajello;L. Baldini
A. A. Abdo;H.D. Aller
N. S. Kardashev;V. V. Khartov;V. V. Abramov;V. Yu. Avdeev
A. A. Abdo;A. A. Abdo;Markus Ackermann;Marco Ajello;A. Allafort
Y. Y. Kovalev;H. D. Aller;M. F. Aller;D. C. Homan
A. B. Pushkarev;Y. Y. Kovalev;Y. Y. Kovalev;M. L. Lister;T. Savolainen
A. A. Abdo;A. A. Abdo;M. Ackermann;M. Ajello;K. Asano
M. L. Lister;M. F. Aller;H. D. Aller;D. C. Homan
T. Savolainen;D.C. Homan;Talvikki Hovatta;Talvikki Hovatta;M. Kadler;M. Kadler;M. Kadler
Y. Y. Kovalev;Y. Y. Kovalev;H. D. Aller;M. F. Aller;D. C. Homan
Alexander B. Pushkarev;Y. Y. Kovalev;Y. Y. Kovalev;M. L. Lister;T. Savolainen;T. Savolainen
Y. Y. Kovalev;Y. Y. Kovalev;M. L. Lister;D. C. Homan;K. I. Kellermann
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