activity
20092023
most citedRadioAstron -- a Telescope with a Size of 300 000 km: Main Parameters and First Observational Results

276 citations · 457 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.IM2023

Processing System for Coherent Dedispersion of Pulsar Radio Emission

Girin I. A., Likhachev S. F., Andrianov A. S. +5

The work describes a system for converting VLBI observation data using the algorithms of coherent dedispersion and compensation of two-bit signal sampling. Coherent dedispersion is…

astro-ph.GA2023★ 6 cited

Technical constraints on interstellar interferometry and spatially resolving the pulsar magnetosphere

M. V. Popov, N. Bartel, A. S. Andrianov +6

Scintillation of pulsar radio signals caused by the interstellar medium can in principle be used for interstellar interferometry. Changes of the dynamic spectra as a function of pu…

astro-ph.GA2022★ 8 cited

Electron density variations in the interstellar medium and the average frequency profile of a scintle from pulsar scintillation spectra

N. Bartel, M. S. Burgin, E. N. Fadeev +4

We observed the scintillation pattern of nine bright pulsars at 324 MHz and three at 1.68 GHz and analyzed the wavenumber spectrum which is related to electron density variations o…

astro-ph.GA2021★ 4 cited

Ionospheric effects in VLBI measured with space-ground interferometer RadioAstron

M. V. Popov, N. Bartel, M. S. Burgin +2

We report on slow phase variations of the response of the space-ground radio interferometer RadioAstron during observations of pulsar B0329+54. The phase variations are due to the…

astro-ph.GA2019★ 13 cited

Substructure of visibility functions from scattered radio emission of pulsars through space VLBI

M. V. Popov, N. Bartel, M. S. Burgin +3

We report on the substructure of visibility functions in the delay domain of PSRs B0329+54, B0823+26, B0834+06, B1933+16 and B0833-45 (Vela) observed with earth-earth and RadioAstr…

astro-ph.HE2016★ 50 cited

PSR B0329+54: Substructure in the scatter-broadened image discovered with RadioAstron on baselines up to 330,000 km

M. V. Popov, N. Bartel, C. R. Gwinn +13

We have resolved the scatter-broadened image of PSR B0329+54 and detected substructure within it. These results are not influenced by any extended structure of a source but instead…