2011 XXXth URSI General Assembly and Scientific Symposium 2011
DOI: 10.1109/ursigass.2011.6123729
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Development of a low-noise wide-band phased-array feed

Abstract: Low-noise phased-array feeds are a new way to expand the field of view of radio telescopes at centimetre wavelengths. First generation engineering demonstrators of this technology have been constructed and tested by several institutes worldwide. The development of second-generation phased-array feeds is now underway. We describe one effort to design and build an astronomy-capable phased-array feed using techniques to reduce front-end noise and increase system bandwidth.

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Cited by 2 publications
(2 citation statements)
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“…The presented LNA achieves lower noise figures than other discrete LNAs and therefore two such LNAs have been installed in one of the 7 Synthesis Telescope antennas operated by the Dominion Radio Astrophysical Observatory (DRAO), National Research Council of Canada. The same LNAs but on a slightly modified PCB have also been used in an Advanced Phased-Array Feed designed by DRAO [10,11].…”
Section: Measured Resultsmentioning
confidence: 99%
“…The presented LNA achieves lower noise figures than other discrete LNAs and therefore two such LNAs have been installed in one of the 7 Synthesis Telescope antennas operated by the Dominion Radio Astrophysical Observatory (DRAO), National Research Council of Canada. The same LNAs but on a slightly modified PCB have also been used in an Advanced Phased-Array Feed designed by DRAO [10,11].…”
Section: Measured Resultsmentioning
confidence: 99%
“…Similar to discussions in Section V-A, numerical analysis was performed on a wide-band 41-element antenna array, known as Advanced Focal Array Demonstrator (AFAD) [41], [42], which is considered as a Square Kilometer Array phasedarray demonstrator [43] and is based on the design in [44]. In this array, the antenna spacing is designed to be half wavelength at 1.5 GHz.…”
Section: B 41-element Antenna Arraymentioning
confidence: 99%