Very Large Array

'Very Large Array' can also refer to...

Very Large Array

Very Large Array

Very Large Array

Karl G. Jansky Very Large Array

An automated archival Very Large Array transients survey

High-resolution Very Large Array observations of 18 MIPSGAL bubbles

The Very Large Array Low-frequency Sky Survey Redux (VLSSr)

Very Large Baseline Array observations of Mrk 6: probing the jet–lobe connection

The Stripe 82 1–2 GHz Very Large Array Snapshot Survey: multiwavelength counterparts

The inner jet of radio galaxy NGC 315 as observed with Chandra and the Very Large Array

A High-Resolution Very Large Array Observation of a Protostar in OMC-3: Shock-Induced X-Ray Emission by a Protostellar Jet

Deep 3-GHz observations of the Lockman Hole North with the Very Large Array – II. Catalogue and μJy source properties

Deep 3-GHz observations of the Lockman Hole North with the Very Large Array – I. Source extraction and uncertainty analysis

The radio–X-ray relation as a star formation indicator: results from the Very Large Array–Extended Chandra Deep Field-South

Tracing the molecular gas in distant submillimetre galaxies via CO(1–0) imaging with the Expanded Very Large Array

Spectral and polarization study of the double relics in Abell 3376 using the Giant Metrewave Radio Telescope and the Very Large Array

On the nature of infrared-faint radio sources in the Subaru X-ray Deep and Very Large Array–VIMOS VLT Deep Survey fields

The eMERGE Survey – I: Very Large Array 5.5 GHz observations of the GOODS-North Field

The Stripe 82 1–2 GHz Very Large Array Snapshot Survey: host galaxy properties and accretion rates of radio galaxies


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An aperture-synthesis radio telescope sited at an altitude of 2124 m on the Plains of San Agustin, west of Socorro, New Mexico, and operated by the US National Radio Astronomy Observatory. It consists of 27 movable dishes of 25-m aperture, mounted along a Y-shaped railway track with arms 19, 21, and 21 km long. The telescopes can be arranged in four different configurations with maximum baselines of 1, 3.6, 10, and 36 km. The data from the antennas is combined electronically to give the resolution of an antenna 36 km across with the sensitivity of a dish 130 m in diameter. The VLA was completed in 1980, and has its headquarters in Socorro, New Mexico. The array is now being upgraded to produce the Expanded Very Large Array (EVLA) with new electronics and up to eight new dishes giving baselines to 350 km.

http://www.vla.nrao.edu/ Official telescope website.

Subjects: Astronomy and Astrophysics.

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