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The Noto VLBI Station is a radio observatory located on Sicily, southern Italy, outside of the city of Noto. The facility is operated by the Istituto di Radioastronomia di Bologna.

The Medicina 32m antenna is located at the Medicina Radio Astronomy Station. The station is run by the Istituto di Radioastronomia and is located about 33 km east of Bologna.

The Mark II is a radio telescope located at Jodrell Bank Observatory, near Goostrey, Cheshire, in the north-west of England.

The 25.6 m diameter, polar mount decimeter-wave telescope in Onsala is equipped with receivers for frequencies up to 7 GHz. The telescope was built in 1963.

The 20 m diameter, radome enclosed, millimetre wave telescope in Onsala is equipped with receivers for frequencies up to 116 GHz. The telescope was built in 1975-76 and upgraded in 1992.

The Plateau de Bure Interferometer (now called NOEMA) is the most advanced facility for milimetre radio astronomy in the Norther hemisphere. The Interferometer will consists of twelve 15-meter antennas and operates with an angular resolution up to 0.1 arcsec.

The 30-metre Telescope on Pico Veleta is the most powerful milimetre single dish telescope in the world.

Metsähovi telescope

The WSRT is one of the most powerful radio observatories in the world. It enables astronomers to study a wide range of astrophysical problems: from pulsars to kinematics of nearby galaxies to the physics of black-holes.

The Atacama Pathfinder Experiment is a modified ALMA prototype antenna operated as a single dish. APEX allows us to observe cold dust and gas in our own Milky Way and in distant galaxies, in the southern sky. This improves our understanding of the structure and chemistry of planetary atmospheres, dying stars, regions of star formation and distant starburst galaxies.