Orbiting very long base interferometer (OVLBI) for radio and optical astronomy

Kardashëv, N. S.; Andreyanov, V. V.; Gvamichava, A. S.; Лихачев, С. Ф.; Slysh, V. I.

doi:10.1016/0094-5765(95)00065-8

Cited by 11 publications

(3 citation statements)

References 6 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…The radio astronomy telescope RT70-Suffa will have the primary reflector with diameter of 70 meters and should be completed in installation on Suffa plateau (not far from Samarqand, Republic of Uzbekistan) at 2350 m altitude (see, e.g., [1] , [2], [3]). Initially this project was designed as a basic part of the Earth-Space VLBI system ( [2], [3]; URL http://www.asc.rssi.ru/suffa/). Spectral bands of the telescope RT70-Suffa will cover wavelength range 0.8-60 mm.…”

Section: Radio Telescope and Radioseeing Projectsmentioning

confidence: 99%

Major Radio Astronomy Telescope RT70-Suffa: Preparation for Future

Hojaev¹

2010

Proceedings of Accelerating the Rate of Astronomical Discovery — PoS(sps5)

View full text Add to dashboard Cite

We briefly outline the Suffa large radio telescope project status and the preparation plan of local radio astronomers. The state-of-art mm-wave radio astronomy telescope having 70m main adaptive reflector will be completed on Suffa plateau in Uzbekistan in the near future. At the moment the steps are making also to further explore the Suffa site 'radioseeing' parameters for the atmosphere modelling at the site and to try to forecast the "radio-weather" for optimal planning the scientific schedule of the future telescope. The multiple step preparation and training of young local radio astronomers who will operate and make a research using this facility are also within our major aims. National University of Uzbekistan(NUU) and the State University of Information Technology(SUIT) will be basic universities for teaching students for these purposes. Naturally all above mentioned together with a broad international collaboration will facilitate for accelerating the rate of astronomical discovery.

show abstract

Section: Radio Telescope and Radioseeing Projectsmentioning

confidence: 99%

Major Radio Astronomy Telescope RT70-Suffa: Preparation for Future

Hojaev¹

2010

Proceedings of Accelerating the Rate of Astronomical Discovery — PoS(sps5)

View full text Add to dashboard Cite

show abstract

“…It should be a basic part of the Earth-Space VLBI system ( Kardashev et al, 1995). With the main instrument similar to the GBT at NRAO it will be one of the main basic elements of the global radio interferometry network as well.…”

Section: Introductionmentioning

confidence: 99%

“…One of the large-scale radio-astronomy facilities is the complex of the International Radio Astronomy Observatory being created on the Suffa plateau (Uzbekistan) in close collaboration with Russia (Kardashev, 1992). It should be a basic part of the Earth-Space VLBI system ( Kardashev et al, 1995). With the main instrument similar to the GBT at NRAO it will be one of the main basic elements of the global radio interferometry network as well.…”

Section: Introductionmentioning

confidence: 99%