activity
20192026
most citedMOJAVE XIX: Brightness Temperatures and Intrinsic Properties of Blazar Jets

102 citations · 192 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.HE2026

Unique Science Opportunities for Space VLBI Systems with the SKA Telescopes

Y. Y. Kovalev, G. Bruni, T. An +17

To date, two dedicated Space Very Long Baseline Interferometry (SVLBI) missions, the VLBI Space Observatory Programme (VSOP) and RadioAstron, have provided groundbreaking insights…

astro-ph.HE2025★ 3 cited

Multi-messenger flare in the quasar PKS 0446+11

Y. Y. Kovalev, M. F. Aller, A. K. Erkenov +15

The physical mechanisms driving neutrino and electromagnetic flares in blazars remain poorly understood. We investigate a prominent multi-messenger flare in the quasar PKS 1424+240…

astro-ph.HE2025★ 3 cited

Dim cores of radio-bright AGN jets: VLBI and Gaia astrometry pinpoint different parsec-scale features

A. V. Popkov, Y. Y. Kovalev, A. V. Plavin +2

Astrometry with the very long baseline radio interferometry (VLBI) allows to determine the position of a point close to the source's brightest compact detail at milliarcsecond scal…

astro-ph.HE2025

Characterizing Candidate Blazar Counterparts of the Ultra-High-Energy Event KM3-230213A

KM3NeT Collaboration, MessMapp Group, LAT Collaboration +13

High-energy astrophysical neutrinos serve as crucial messengers for understanding hadronic acceleration processes and identifying the origins of cosmic rays, with blazars among the…

astro-ph.HE2024★ 10 cited

Multiwavelength variability of the blazar AO 0235+164

V. V. Vlasyuk, Yu. V. Sotnikova, A. E. Volvach +28

We present a study of the multiwavelength (MW) variability of the blazar AO 0235+164 based on the radio-to--ray data covering a long time period from 1997 to 2023. The radio dat…

astro-ph.HE2024★ 15 cited

A wiggling filamentary jet at the origin of the blazar multi-wavelength behaviour

C. M. Raiteri, M. Villata, M. I. Carnerero +96

Blazars are beamed active galactic nuclei known for their strong multi-wavelength variability on timescales from years down to minutes. We aim to investigate the suitability of the…

astro-ph.HE2023★ 9 cited

Multi-band Cross-correlated Radio Variability of the Blazar 3C 279

Krishna Mohana A, Alok C. Gupta, Alan P. Marscher +18

We present the results of our study of cross-correlations between long-term multi-band observations of the radio variability of the blazar 3C 279. More than a decade (2008-2022) of…

astro-ph.HE2023

Baikal-GVD Astrophysical Neutrino Candidate near the Blazar TXS~0506+056

V. M. Aynutdinov, V. A. Allakhverdyan, A. D. Avrorin +71

We report on the observation of a rare neutrino event detected by Baikal-GVD in April 2021. The event GVD210418CA is the highest-energy cascade observed by Baikal-GVD so far from t…

astro-ph.HE2022★ 25 cited

High-energy neutrino-induced cascade from the direction of the flaring radio blazar TXS 0506+056 observed by Baikal-GVD in 2021

GVD Collaboration, A. K. Erkenov, N. A. Kosogorov +8

The existence of high-energy astrophysical neutrinos has been unambiguously demonstrated, but their sources remain elusive. IceCube reported an association of a 290-TeV neutrino wi…

astro-ph.HE2021★ 102 cited

MOJAVE XIX: Brightness Temperatures and Intrinsic Properties of Blazar Jets

D. C. Homan, M. H. Cohen, T. Hovatta +7

We present multi-epoch, parsec-scale core brightness temperature observations of 447 AGN jets from the MOJAVE and 2cm Survey programs at 15 GHz from 1994 to 2019. The brightness te…

astro-ph.GA2020★ 18 cited

Parsec-scale properties of steep and flat spectrum extragalactic radio sources from a VLBA survey of a complete north polar cap sample

Alexander V. Popkov, Yuri Y. Kovalev, Leonid Y. Petrov +1

We observed with the VLBA at 2.3 and 8.6 GHz a complete flux-density limited sample of 482 radio sources with declination >+75 degrees brighter than 200 mJy at 1.4 GHz drawn from t…

astro-ph.EP2019★ 7 cited

The Rate of Planet-star Coalescences Due to Tides and Stellar Evolution

Alexander V. Popkov, Sergei B. Popov

Orbits of close-in planets can shrink significantly due to dissipation of tidal energy in a host star. This process can result in star-planet coalescence within the Galactic lifeti…