RT-22 LPI Radio Telescope - is a parabolic reflector with its main dish of 22m in diameter. Accuracy of the main dish surface provides telescope's effective operation up to mm wavelengths. The telescope's receivers have the latest cooled low noise preamplifiers. The major scientific programs deal with star formation regions research by observations of atomic and molecular radio lines, and investigations of compact radio sources structures using interferometer technique with the resolution of hundredth and thousandth part of arcsecond.

  BSA LPI Radio Telescope - is a phased array comprising 16384 dipoles and covering an area of 18 acres. Its operating wavelength is 3m, and the telescope is world's most sensitive instrument in the range. BSA LPI is an indispensable one for the whole series dynamic processes in the near-Sun and interplanetary plasma, studies of pulsar radio emission, and analysis of the compact radio sources structure in the meter range of wavelengths.