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most citedCompact radio emission indicates a structured jet was produced by a binary neutron star merger

395 citations · 2.7k across the 108 of their papers we have counts for

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astro-ph2008★ 5 cited

The Apparent "Angular Size - Frequency" Dependence in ~3000 Parsec-scale Extragalactic Jets

J. Yang, L. I. Gurvits, S. Frey +1

The upper envelope of the amplitude of the VLBI visibility function usually represents the most compact structural pattern of extragalactic radio sources, in particular, the "core-…

astro-ph2008★ 45 cited

High-resolution double morphology of the most distant known radio quasar at z=6.12

S. Frey, L. I. Gurvits, Z. Paragi +1

Context: The highest redshift quasars at z>~6 receive considerable attention since they provide strong constraints on the growth of the earliest supermassive black holes. They also…

astro-ph2008

High-Redshift Quasars at the Highest Resolution: VSOP Results

S. Frey, L. I. Gurvits, A. P. Lobanov +2

We studied the radio structure of high-redshift (z>3) quasars with VSOP at 1.6 and 5 GHz. These sources are the most distant objects ever observed with Space VLBI, at rest-frame fr…

astro-ph2007★ 15 cited

Deep Extragalactic VLBI-Optical Survey (DEVOS) II. Efficient VLBI detection of SDSS quasars

S. Frey, L. I. Gurvits, Z. Paragi +3

Context: The Deep Extragalactic VLBI-Optical Survey (DEVOS) aims at constructing a large sample of compact radio sources up to two orders of magnitude fainter than those studied in…

astro-ph2006

The VSOP Survey: Final individual results + Final aggregate results

R. Dodson, S. Horiuchi, W. Scott +10

In February 1997 the Japanese radio astronomy satellite HALCA was launched to provide the space-borne element for the VSOP mission. HALCA provided linear baselines three-times grea…

astro-ph2006

Dual-frequency VSOP Imaging of a High-redshift Radio Quasar PKS 1402+044

Jun Yang, Leonid Gurvits, Andrei Lobanov +2

Based on the VLBI Space Observatory Programme (VSOP) observations at 1.6 and 5 GHz, we find that the luminous high-redshift (z=3.215) quasar PKS 1402+044 (J1405+0415) has a pronoun…