Angular structure of extragalactic radio sources at low frequencies
The low frequency VLBI of URAN network operated in the decameter range has been designed in Ukraine to study cosmic radio sources. The network consists of five radio telescopes making up of four interferometers with baselines range from 42 to 913 km with UTR-2 radio telescope operated as the main a...
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| Опубліковано в: : | Кинематика и физика небесных тел |
|---|---|
| Дата: | 2005 |
| Автори: | , , , , , |
| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
Головна астрономічна обсерваторія НАН України
2005
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| Теми: | |
| Онлайн доступ: | https://nasplib.isofts.kiev.ua/handle/123456789/79601 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Цитувати: | Angular structure of extragalactic radio sources at low frequencies / A.I. Brazhenko, V.V. Koshovy, A.R. Lozynsky, A.V. Megn, S.L. Rashkovsky, V.A. Shepelev // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 47-50. — Бібліогр.: 2 назв. — англ. |
Репозитарії
Digital Library of Periodicals of National Academy of Sciences of Ukraine| id |
nasplib_isofts_kiev_ua-123456789-79601 |
|---|---|
| record_format |
dspace |
| spelling |
Brazhenko, A.I. Koshovy, V.V. Lozynsky, A.R. Megn, A.V. Rashkovsky, S.L. Shepelev, V.A. 2015-04-03T15:01:46Z 2015-04-03T15:01:46Z 2005 Angular structure of extragalactic radio sources at low frequencies / A.I. Brazhenko, V.V. Koshovy, A.R. Lozynsky, A.V. Megn, S.L. Rashkovsky, V.A. Shepelev // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 47-50. — Бібліогр.: 2 назв. — англ. 0233-7665 https://nasplib.isofts.kiev.ua/handle/123456789/79601 The low frequency VLBI of URAN network operated in the decameter range has been designed in Ukraine to study cosmic radio sources. The network consists of five radio telescopes making up of four interferometers with baselines range from 42 to 913 km with UTR-2 radio telescope operated as the main antenna of the interferometers. The angular resolution of the network amount to 1 arcsec at the highest frequency of the range, and its sensitivity is about 20 Jy. Regular observations of galactic and extragalactic radio sources are performed with the network. Some results of studies are presented here. en Головна астрономічна обсерваторія НАН України Кинематика и физика небесных тел MS1: Decameter Radioastronomy Angular structure of extragalactic radio sources at low frequencies Article published earlier |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
Angular structure of extragalactic radio sources at low frequencies |
| spellingShingle |
Angular structure of extragalactic radio sources at low frequencies Brazhenko, A.I. Koshovy, V.V. Lozynsky, A.R. Megn, A.V. Rashkovsky, S.L. Shepelev, V.A. MS1: Decameter Radioastronomy |
| title_short |
Angular structure of extragalactic radio sources at low frequencies |
| title_full |
Angular structure of extragalactic radio sources at low frequencies |
| title_fullStr |
Angular structure of extragalactic radio sources at low frequencies |
| title_full_unstemmed |
Angular structure of extragalactic radio sources at low frequencies |
| title_sort |
angular structure of extragalactic radio sources at low frequencies |
| author |
Brazhenko, A.I. Koshovy, V.V. Lozynsky, A.R. Megn, A.V. Rashkovsky, S.L. Shepelev, V.A. |
| author_facet |
Brazhenko, A.I. Koshovy, V.V. Lozynsky, A.R. Megn, A.V. Rashkovsky, S.L. Shepelev, V.A. |
| topic |
MS1: Decameter Radioastronomy |
| topic_facet |
MS1: Decameter Radioastronomy |
| publishDate |
2005 |
| language |
English |
| container_title |
Кинематика и физика небесных тел |
| publisher |
Головна астрономічна обсерваторія НАН України |
| format |
Article |
| description |
The low frequency VLBI of URAN network operated in the decameter range has been designed in Ukraine to study cosmic radio sources. The network consists of five radio telescopes making up of four interferometers with baselines range from 42 to 913 km with UTR-2 radio telescope operated as the main antenna of the interferometers. The angular resolution of the network amount to 1 arcsec at the highest frequency of the range, and its sensitivity is about 20 Jy. Regular observations of galactic and extragalactic radio sources are performed with the network. Some results of studies are presented here.
|
| issn |
0233-7665 |
| url |
https://nasplib.isofts.kiev.ua/handle/123456789/79601 |
| citation_txt |
Angular structure of extragalactic radio sources at low frequencies / A.I. Brazhenko, V.V. Koshovy, A.R. Lozynsky, A.V. Megn, S.L. Rashkovsky, V.A. Shepelev // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 47-50. — Бібліогр.: 2 назв. — англ. |
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AT brazhenkoai angularstructureofextragalacticradiosourcesatlowfrequencies AT koshovyvv angularstructureofextragalacticradiosourcesatlowfrequencies AT lozynskyar angularstructureofextragalacticradiosourcesatlowfrequencies AT megnav angularstructureofextragalacticradiosourcesatlowfrequencies AT rashkovskysl angularstructureofextragalacticradiosourcesatlowfrequencies AT shepelevva angularstructureofextragalacticradiosourcesatlowfrequencies |
| first_indexed |
2025-12-07T13:35:15Z |
| last_indexed |
2025-12-07T13:35:15Z |
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