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.

FCRAO focuses on the study of objects which are now familiar and attempt to learn their secrets. The future platform is the Large Millimeter Telescope/Gran Telescopio Milimetrico (LMT/GTM), a project to construct and operate a 50 meter telescope between 1 and 3mm. Offers research and contact information.

NASA's worldwide antenna network to support the exploration of the solar system.

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.

Site provides educational information about radio astronomy. Radiotelescope data from their project is posted on the Web in real time.

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.

MRT is a 2km x 1km T-shaped aperture synthesis array consisting of 1024 fixed 2m helical antennae and 64 moveable arrays. Offers information on the observaroty, activities, research, photographs 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.