The maximum signal bandwidth on the Australia Telescope Compact Array (ATCA) is to expand from 128MHz to 2GHz. Central to this development is a Field Programmable Gate Array (FPGA)-based digital filterbank correlator featuring high dynamic range and flexible configuration. Associated analog to digital conversion requirements will push the limits of high-speed sampling and quantisation techniques. These new technologies are direct candidates for signal processing on the proposed Square Kilometer Array (SKA). The correlator includes extra ports to incorporate two SKA demonstrator antenna stations into the ATCA, providing both a more powerful instrument and a mature test bed for the demonstrators. OVERVIEW The Australia Telescope Compact Array...
An FPGA-based digital-receiver has been developed for a low-frequency imaging radio interferometer, ...
The Atacama Large Millimeter Array (ALMA) is a single astronomical instrument consisting of up to 64...
The Square Kilometre Array radio telescope (SKA) will be a next generation radio telescope, 100 to 1...
Here, we describe the Compact Array Broad-band Backend (CABB) and present first results obtained wit...
Here, we describe the Compact Array Broad-band Backend (CABB) and present first results obtained wit...
The Long Baseline Array (LBA) is the only astronomical VLBI array operating in the southern hemisphe...
Restricted Access.Here, we describe the Compact Array Broad-band Backend (CABB) and present first re...
Here, we describe the Compact Array Broad‐band Backend (CABB) and present first results obtained wit...
Here, we describe the Compact Array Broad‐band Backend (CABB) and present first results obtained wit...
The radio astronomy community is engaged in the development of the Square Kilometre Array (SKA). The...
The definitive version can be found at: http://onlinelibrary.wiley.com/ Copyright Royal Astronomical...
Current attempts to make precision measurements of the HI power spectrum at high redshifts have led ...
The radio astronomy community is engaged in the development of the Square Kilometre Array (SKA). The...
ABSTRACT: We propose to use funds from the GBT azimuth track remediation settlement for two projects...
Abstract — The Molonglo radio telescope near Canberra, Australia, is an east-west array of two colli...
An FPGA-based digital-receiver has been developed for a low-frequency imaging radio interferometer, ...
The Atacama Large Millimeter Array (ALMA) is a single astronomical instrument consisting of up to 64...
The Square Kilometre Array radio telescope (SKA) will be a next generation radio telescope, 100 to 1...
Here, we describe the Compact Array Broad-band Backend (CABB) and present first results obtained wit...
Here, we describe the Compact Array Broad-band Backend (CABB) and present first results obtained wit...
The Long Baseline Array (LBA) is the only astronomical VLBI array operating in the southern hemisphe...
Restricted Access.Here, we describe the Compact Array Broad-band Backend (CABB) and present first re...
Here, we describe the Compact Array Broad‐band Backend (CABB) and present first results obtained wit...
Here, we describe the Compact Array Broad‐band Backend (CABB) and present first results obtained wit...
The radio astronomy community is engaged in the development of the Square Kilometre Array (SKA). The...
The definitive version can be found at: http://onlinelibrary.wiley.com/ Copyright Royal Astronomical...
Current attempts to make precision measurements of the HI power spectrum at high redshifts have led ...
The radio astronomy community is engaged in the development of the Square Kilometre Array (SKA). The...
ABSTRACT: We propose to use funds from the GBT azimuth track remediation settlement for two projects...
Abstract — The Molonglo radio telescope near Canberra, Australia, is an east-west array of two colli...
An FPGA-based digital-receiver has been developed for a low-frequency imaging radio interferometer, ...
The Atacama Large Millimeter Array (ALMA) is a single astronomical instrument consisting of up to 64...
The Square Kilometre Array radio telescope (SKA) will be a next generation radio telescope, 100 to 1...