[alfazoOm] is basing his telescope off of the Stony Brook radio interferometer, though he is designing custom hardware that can position the dish in whatever direction the operator desires with an ...

The Owens Valley Long Wavelength Array (OVRO-LWA) is a low-frequency radio interferometer composed of 288 crossed broadband dipole antennas. The OVRO-LWA band covers 58 MHz of instantaneous bandwidth ...

As noted, COSMIC will compute 64 synthetic beams on the sky (all falling within the wide, single beam of an individual antenna), using well-known techniques of radio interferometry. These beams are ...

However, instead of building increasingly large dishes, which becomes more difficult and expensive, radio interferometry replaces the single dish with many smaller dishes, and connects them together ...

The Owens Valley Long Wavelength Array (OVRO-LWA) is a low-frequency radio interferometer composed of 288 crossed broadband dipole antennas. The OVRO-LWA band covers 58 MHz of instantaneous bandwidth ...

In radio astronomy, tripole antennas find an application in space telescopes. More recently, a radio interferometer with satellite-borne tripole antennas is being considered for a lunar orbiting radio ...

Publications of the Astronomical Society of the Pacific, Vol. 134, No. 1040 (2022 October), pp. 1-12 (12 pages) Correlation for radio interferometer array applications, including Very Long Baseline ...