Astronomy: Institutions: Observatories: Radio

A 10.4-meter diameter, submillimeter spectrum telescope. Situated at the top of Mauna Kea, Big island, Hawaii.

This is the main page for the Berkeley-Illinois-Maryland Association (BIMA)

Part of the School of Natural Sciences of the Tata Institute of Fundamental Research, includes information on observing with a Giant Metrewave Radio Telescope, research opportunities, job openings, library, staff, observing facilities, Ooty Radio Telescope and contact details.

The largest radio telescope in the world.

This Kraus-type radio telescope, larger than three football fields, was famous for the Wow! Signal and for the longest-running SETI project.

The core of the Centre for Astrophysics and Space Science, includes research interests in basic astrophysics through observational astronomy, and especially technical research is in sensitive low-noise millimetre/radio wave receiver techniques for applications in ground- or space-based sensors. Offers information on publications, activities, research, education and contact details.

Research involving the study of stellar, interstellar, and extragalactic radio emission. Major projects include the Canadian Galactic Plane Survey, the VLA Galactic Plane Survey, Space Very Long Baseline Interferometry, the Square Kilometer Array, the Canadian Large Adaptive Reflector, and Karma Astronomical Visualization Software. Information on staff research, related facilites, education and contact details.

Manages a broad program of research, including the Mullard Radio Astronomy Observatory, situated at Lord's Bridge. Information on group members, research interests, publications, surveys and catalogues, other resources.

MOST is operated by the School of Physics, University of Sydney, and consists of two cylindrical paraboloids, 778m x 12m, separated by 15m and aligned East-West. A line feed system of 7744 circular dipoles collects the signal and feeds 176 preamplifiers and 88 IF amplifiers. Includes student and research information, documents and contact details.

An array of radio telescopes, a solar interferometer, and other instruments are available to astronomers at this observatory, located near Big Pine, California.

Operates the Australia Telescope, a set of radio telescopes in New South Wales. These telescopes are used, individually or together, to study objects in the Universe ranging from the remains of dead stars to entire galaxies.

NRAL at Jodrell Bank are a part of the University of Manchester's Department of Physics and Astronomy. The Laboratories are home to the Lovell Telescope and the MERLIN & VLBI National Facility which is operated by the University on behalf of PPARC.

in Tenerife (Canary Islands). Designed to study fluctuations in the Cosmic Microwave Background (CMB) thought to originate from the period immediately following the big bang. Operated by Cambridge and Manchester Universities (UK).

Research facility of National Science Foundation, operates many radio telescope observatories.

An array with a collecting area of up to 10,000 square meters. With baselines foreseen to extend to 10 Km, the angular resolution provided by the new instrument will be that of a diffraction limited 4m optical telescope.

An eight element submillimeter interferometer being constructed on the summit of Mauna Kea in Hawaii.

A 36-km diameter radio telescope consisting of 27 individual dishes arranged in a Y shape. Featured in the films 2001 and Contact (the latter half).

Information on the telescope, research projects, observation results, weather, documentation, schedule and contact details.

JIVE was created by the European Consortium for VLBI and its primary task is to operate the EVN MkIV VLBI Data Processor (correlator) as well as provides a high-level of support to astronomers and the Telescope Network. JIVE is hosted by the Netherlands Foundation for Research in Astronomy. Offers information on research, and contact information.