Library · IAA RAS

Papers

Blazar Observations at the RT-32 Radio Telescope of the IAA RAS Svetloe Observatory

A. A. Arkharov, I. A. Rakhimov, D. V. Ivanov, A. V. Ipatov, V. M. Larionov, T. S. Andreeva

Transactions of IAA RAS, issue 51, 13–19 (2019)

Keywords: blazars, active galactic nuclei, flux density, radio telescope, spectrum

Abstract

The first observational results obtained at the Svetloe Observatory of the IAA RAS under the WEBT — World Blazar Telescope project [1-2] are presented. This international project, led by Italian astronomers, combines the efforts of observatories around the world and is aimed at a comprehensive study of the active nuclei of galaxies in the entire range of the electromagnetic spectrum, from radio waves to gamma radiation. The Svetloe Observatory joined the project in March 2018 and since then has been conducting regular observations as the part of the “Scale” program on the RT-32 telescope at frequencies of 4.8 and 8.5 GHz. The first results of measuring the flux density at the frequencies given above were obtained for several objects. The results of monitoring the radio flux density of the blazar 3C 279, being one of the most active sources of this type, are discussed. These data were transmitted to the Torino Observatory and will be used within the WEBT project.

Citation

Text

BibTeX

RIS

A. A. Arkharov, I. A. Rakhimov, D. V. Ivanov, A. V. Ipatov, V. M. Larionov, T. S. Andreeva. Blazar Observations at the RT-32 Radio Telescope of the IAA RAS Svetloe Observatory // Transactions of IAA RAS. — 2019. — Issue 51. — P. 13–19.

@article{arkharov2019,
  abstract = {The first observational results obtained at the Svetloe Observatory of the IAA RAS under the WEBT — World Blazar Telescope project [1-2] are presented.
This international project, led by Italian astronomers, combines the efforts of observatories around the world and is aimed at a comprehensive study of the active nuclei of galaxies in the entire range of the electromagnetic spectrum, from radio waves to gamma radiation. The Svetloe Observatory joined the project in March 2018 and since then has been conducting regular observations as the part of the “Scale” program on the RT-32 telescope at frequencies of 4.8 and 8.5 GHz. The first results of measuring the flux density at the frequencies given above were obtained for several objects. The results of monitoring the radio flux density of the blazar 3C 279, being one of the most active sources of this type, are discussed. These data were transmitted to the Torino Observatory and will be used within the WEBT project.},
  author = {A.~A. Arkharov and I.~A. Rakhimov and D.~V. Ivanov and A.~V. Ipatov and V.~M. Larionov and T.~S. Andreeva},
  doi = {10.32876/ApplAstron.51.13-19},
  issue = {51},
  journal = {Transactions of IAA RAS},
  keyword = {blazars, active galactic nuclei, flux density, radio telescope, spectrum},
  pages = {13--19},
  title = {Blazar Observations at the RT-32 Radio Telescope of the IAA RAS Svetloe Observatory},
  url = {http://iaaras.ru/en/library/paper/2005/},
  year = {2019}
}

TY  - JOUR
TI  - Blazar Observations at the RT-32 Radio Telescope of the IAA RAS Svetloe Observatory
AU  - Arkharov, A. A.
AU  - Rakhimov, I. A.
AU  - Ivanov, D. V.
AU  - Ipatov, A. V.
AU  - Larionov, V. M.
AU  - Andreeva, T. S.
PY  - 2019
T2  - Transactions of IAA RAS
IS  - 51
SP  - 13
AB  - The first observational results obtained at the Svetloe Observatory
of the IAA RAS under the WEBT — World Blazar Telescope project [1-2]
are presented.  This international project, led by Italian
astronomers, combines the efforts of observatories around the world
and is aimed at a comprehensive study of the active nuclei of
galaxies in the entire range of the electromagnetic spectrum, from
radio waves to gamma radiation. The Svetloe Observatory joined the
project in March 2018 and since then has been conducting regular
observations as the part of the “Scale” program on the RT-32
telescope at frequencies of 4.8 and 8.5 GHz. The first results of
measuring the flux density at the frequencies given above were
obtained for several objects. The results of monitoring the radio
flux density of the blazar 3C 279, being one of the most active
sources of this type, are discussed. These data were transmitted to
the Torino Observatory and will be used within the WEBT project.
DO  - 10.32876/ApplAstron.51.13-19
UR  - http://iaaras.ru/en/library/paper/2005/
ER  -