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Astronomical interferometer

An astronomical interferometer or telescope array is a set of separate telescopes, mirror segments, or radio telescope antennas that work together as a single telescope to provide higher resolution images of astronomical objects such as stars, nebulas and galaxies by means of interferometry. The advantage of this technique is that it can theoretically produce images with the angular resolution of a huge telescope with an aperture equal to the separation, called baseline, between the component telescopes.

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Allen Telescope Array

The Allen Telescope Array (ATA), formerly known as the One Hectare Telescope (1hT), is a radio telescope array dedicated to astronomical observations and a simultaneous search for extraterrestrial intelligence (SETI).

Hooker telescope

Laser Interferometer Space Antenna

The Laser Interferometer Space Antenna (LISA) is a planned space probe to detect and accurately measure gravitational waves-tiny ripples in the fabric of spacetime-from astronomical sources.

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Quantum computing is a rapidly developing field that utilizes principles of quantum mechanics to process and store information.

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Radio astronomy is a subfield of astronomy that studies celestial objects at radio frequencies.

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A radio telescope is a specialized antenna and radio receiver used to detect radio waves from astronomical radio sources in the sky.

Reflecting telescope

A reflecting telescope (also called a reflector) is a telescope that uses a single or a combination of curved mirrors that reflect light and form an image.