The radio telescope located in Brewster is one of ten dishes comprising the Very Long Baseline Array.

The radio telescope at the Observatory is one of ten dishes comprising the Very Long Baseline Array (VLBA).

But no superluminal motion has been detected, despite frequent monitoring by the Very Long Baseline Array (VLBA).

Together, the 10 make up the National Radio Astronomy Observatory's Very Long Baseline Array and make up a single radio telescope.

Measurements using the Very Long Baseline Array in 2009 found velocities as large as 254 km/s for stars at the outer edge of the Milky Way.

One of the ten dish antennas of the Very Long Baseline Array is immediately adjacent to, but not part of, the observatory.

In 2010 this dish was used for several Very Long Baseline Interferometry observations as part of the Australian Long Baseline Array.

The observations were made by the Very Long Baseline Array, a system of 10 identical radiotelescope antennas ranging from Hawaii to the Virgin Islands.

It identifies construction of the Very Long Baseline Array as a priority.

Observations in 2004 by the Very Long Baseline Array for 42 consecutive days gave new data and understanding of the action of the jets.