interferometric

This will be possible through a technique known as interferometric observations.

It forms the basis of the self-calibration approach to interferometric imaging.

This is the largest optical interferometric array ever built.

This was the first interferometric measurement of any object outside the Solar System.

Interferometric observations give a radius that is about 173% that of the Sun.

By using interferometric techniques, nanometer changes can be detected.

A detailed discussion on interferometric autocorrelation is given in several well-known textbooks.

Any attempt to intercept the signal causes the collapse of the interferometric pattern.

As of 2005, four of the six telescopes have been commissioned for interferometric observations.

There is a Coudé focus provided for there interferometric array.

Robert Forward operated an interferometric detector at Hughes in the early 1970s.

First a typical interferometric detector will be described.

In the infrared, the array has an interferometric imaging resolution of 0.0005 arcseconds.

As with many interferometric techniques, it is not possible to identify the zero-order fringe without additional information from the system.

At the time it was built, it was world's largest interferometric array.

Optical interferometric measurements require high sensitivity, low noise detectors that did not become available until the late 1990s.

The interferometric and spectroscopic observations allow the distance to the system to be determined independently of other methods.

Do you have the interferometric position?

The project is based on an interferometric array of radio telescopes using about 25,000 small antennas concentrated in at least 48 larger stations.

This nominal length is known as the interferometric length.

It is estimated to have about 50% more mass than the Sun, while interferometric measurements show it to be 15 times larger in diameter.

With advances in interferometric methodologies, astronomers may be close to resolving this conundrum.

Binary stars which can be resolved with a telescope or interferometric methods are known as visual binaries.

The first case considered the mixing of neutral mesons, because their interferometric nature makes them highly sensitive to suppressed effects.

Interferometers and interferometric techniques may be categorized by a variety of criteria: