Abstract The Arcminute Microkelvin Imager (AMI) telescopes located at the Mullard Radio
Astronomy Observatory near Cambridge have been significantly enhanced by the …

We describe the design, validation, and commissioning of a new correlator termed
'MWAX'for the Murchison Widefield Array (MWA) low-frequency radio telescope. MWAX …

An FPGA-based digital-receiver has been developed for a low-frequency imaging radio
interferometer, the Murchison Widefield Array (MWA). The MWA, located at the Murchison …

The Murchison Widefield Array is a new low-frequency interferometric radio telescope built
in Western Australia at one of the locations of the future Square Kilometre Array. We …

The Murchison Widefield Array (MWA) is one of three Square Kilometre Array Precursor
telescopes and is located at the Murchison Radio-astronomy Observatory in the Murchison …

The Murchison Widefield Array is a Square Kilometre Array Precursor. The telescope is
located at the Murchison Radio–astronomy Observatory in Western Australia. The MWA …

The science cases for incorporating high time resolution capabilities into modern radio
telescopes are as numerous as they are compelling. Science targets range from exotic …

Electron Multiplying Charge Coupled Devices (EMCCDs) are CCD cameras with potentially
single-photon detection ability. Signal amplification is achieved by way of a unique electron …

The improved High-resolution Fast Imager (HiFI+) is a multiwavelength imaging filtergraph,
which was commissioned at the GREGOR solar telescope at Observatorio del Teide, Izaña …

Aims. We describe a 6–12 GHz analogue correlator that has been developed for use in
radio interferometers. Methods. We use a lag-correlator technique to synthesis eight …