Very Large Array

The Karl G. Jansky Very Large Array is a centimeter-wavelength radio astronomy observatory located in central New Mexico on the Plains of San Agustin, between the towns of Magdalena and Datil, ~50 miles west of Socorro. The VLA comprises twenty-eight 25-meter radio telescopes deployed in a Y-shaped array and all the equipment, instrumentation, and computing power to function as an interferometer. Each of the massive telescopes is mounted on double parallel railroad tracks, so the radius and density of the array can be transformed to adjust the balance between its angular resolution and its surface brightness sensitivity. Astronomers using the VLA have made key observations of black holes and protoplanetary disks around young stars, discovered magnetic filaments and traced complex gas motions at the Milky Way's center, probed the Universe's cosmological parameters, and provided new knowledge about the physical mechanisms that produce radio emission.

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SETI Researchers can now Scan all Data at the Very Large Array for any Evidence of Alien Transmissions

COSMIC: All Antennas at the Very Large Array Ready to Stream Data for Technosignature Research

COSMIC: All antennas at the Very Large Array ready to stream data for technosignature research