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Channel: Techniques – MIT Kavli Institute
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Radio Astronomy

The MIT Kavli Institute is a partner in the Murchison Widefield Array (MWA) project, a low frequency radio array under construction in Western Australia. The MWA is made up of 128 antenna “tiles,” 4X4...

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Precision Measurement

Advanced quantum noise reduction squeezed light and filter cavities The quantum nature of light presents a limit to the precision of optical measurements. In the case of a gravitational wave detector,...

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Planetary Remote Sensing

Microwave MKI supplied the PI for the Magellan Venus radar mapping mission (1990-94) and was responsible for the analysis of altimetry and radiometry data. This resulted in what are currently the most...

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Pencil & Paper

Researchers at MKI work on a broad range of topics in theoretical astrophysics. Ed Bertschinger group: formation of cosmic structure, the physics of dark matter, the physics of gravitation, and the...

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Particle Astrophysics

These particles can be studies directly with detectors in space, on the ground, or underground. They can also be studied by the products of their interactions, which can happen locally with the Earth...

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Optical/IR Astronomy

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High Performance Computing

Scott Hughes Group Modeling of gravitational-wave sources and their measurement by gravitational-wave detectors.  Modeling sources requires solving the equations of generic relativity to high accuracy,...

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High Energy Astrophysics

MKI has been and continues to be involved in instrumentation for a variety of space-based high-energy astrophysics missions including the Advanced CCD imaging Spectrometer (ACIS) and High-Energy...

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Gravitational Wave Detection

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