A low frequency radio telescope at mauritius for a southern sky survey

被引:0
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作者
K. Golap
N. Udaya Shankar
S. Sachdev
R. Dodson
Ch. V. Sastry
机构
[1] University of Mauritius,Departments of Physics
[2] Raman Research Institute,Physics Department
[3] Indian Institute of Astrophysics,undefined
[4] University of Durham,undefined
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关键词
Radio telescope; low frequency; imaging; southern sky; Fourier Synthesis;
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摘要
A new, meter-wave radio telescope has been built in the north-east of Mauritius, an island in the Indian Ocean, at a latitude of -20.14‡. The Mauritius Radio Telescope (MRT) is a Fourier Synthesis T-shaped array, consisting of a 2048 m long East-West arm and an 880 m long South arm. In the East-West arm 1024 fixed helices are arranged in 32 groups and in the South arm 16 trolleys, with four helices on each, which move on a rail are used. A 512-channel digital complex correlation receiver is used to measure the visibility function. At least 60 days of observing are required for obtaining the visibilities up to 880 m spacing. The Fourier transform of the calibrated visibilities produces a map of the area of the sky under observation with a synthesized beam width 4′ × 4.6′ sec(δ + 20.14‡) at 151.5 MHz.
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页码:35 / 53
页数:18
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