  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 deg. The
Mauritius Radio Telescope (MRT) is a Fourier Synthesis T-shaped array,
consisting of a 2048 m long East-West arm and a 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'X 4.6'sec(dec+20.14) at 151.5 MHz.
  The primary objective of the telescope is to produce a sky survey in the
declination range -70 deg to -10 deg with a point source sensitivity of about
200 mJy (3-sigma level). This will be the southern sky equivalent of the
Cambridge 6C survey. In this paper we describe the telescope, discuss the array
design and the calibration techniques used, and present a map made using the
telescope.
