The above image shows uv-coverage for a configuration where the antennas are placed at the nodes of the Sierpinski Gasket (Fractal). I strongly suggest that we use this configuration for our proposed radio telescope in the institute.

Consider any point on the ground as reference and then the coordinates of the antennas are the following:

X (E)	Y (N)
4.500000	23.382675
18.000000	0.000000
-9.000000	0.000000
0.000000	15.588450

All distances are in meters. The X-axis is along the East direction and the Y-axis along the North direction.