Overview
The Sardinia Radio Telescope (SRT) is a 64-meter diameter parabolic radio telescope operated by the Italian National Institute for Astrophysics (INAF) and managed by the Astronomical Observatory of Cagliari.
It is situated in the plain of Pranu Sanguni in San Basilio at an altitude of 600 m a.s.l., 35 km north of Cagliari (IT). One of the most advanced technical features of the SRT is its active surface, comprising 1008 aluminium panels supported by electromechanical actuators in order to compensate for deformations induced by gravity and allowing us to observe a wide range of scientific targets from 300 MHz to 116 GHz.
SRT operates both as a single dish (continuum, full Stokes, timing and spectroscopy) and as part of European and international networks (Very Long Baseline Interferometry and Pulsar Timing networks), participating in regular calls for proposals.
Thanks to its large aperture and versatility (multi-frequency agility and wide frequency coverage), SRT is dedicated to achieving scientific excellence, providing open access to the research community, and fostering public engagement through education and outreach initiatives.
Learn More About Us