The Sardinia Radio Telescope (SRT) is 64-metre fully steerable radio telescope near
San Basilio,
Province of Cagliari,
Sardinia
Sardinia ( ; ; ) is the Mediterranean islands#By area, second-largest island in the Mediterranean Sea, after Sicily, and one of the Regions of Italy, twenty regions of Italy. It is located west of the Italian Peninsula, north of Tunisia an ...
, Italy. Completed in 2011, it is a collaboration between the
Istituto di Radioastronomia di Bologna, the
Cagliari Observatory (Cagliari) and the
Arcetri Astrophysical Observatory (Florence).
Design

The telescope is in Sardinia, north of
Cagliari
Cagliari (, , ; ; ; Latin: ''Caralis'') is an Comune, Italian municipality and the capital and largest city of the island of Sardinia, an Regions of Italy#Autonomous regions with special statute, autonomous region of Italy. It has about 146,62 ...
,
and is the largest
of a set of three telescopes operated by
INAF, along with telescopes at the
Medicina Radio Observatory and the
Noto Radio Observatory. It operates as a stand-alone instrument and as part of global networks of telescopes. The telescope and its structure weighs around .
The primary mirror is in diameter. It has an
active surface consisting of 1008 aluminum panels in 14 rows. Each panel has an area between 2.4 and 5.3 square metres. There are 1116 actuators mounted on the backing structure, which move the surface panels to correct for the distortion of the mirror with elevation. A quadrupod supports a diameter subreflector, with 49 panels in three rows, as well as primary focus instrumentation.
The telescope is fully steerable. The telescope sits on a reinforced concrete base, carved into bedrock, with a continuously-welded track sitting on a diameter outer ring, connected to the foundations with 260 pairs of anchor bolts, and supporting 16 wheels. In the centre is the azimuth bearing support, as well as the cable wrap and encoder system. The welded steel
alidade
An alidade () (archaic forms include alhidade, alhidad, alidad) or a turning board is a device that allows one to sight a distant object and use the line of sight to perform a task. This task can be, for example, to Triangulation (surveying), tr ...
then supports the elevation wheel, which is in turn connected to the primary mirror backing structure. A room at the base of the alidade holds the motor power supplies, antenna control system, and cryogenic compressors. Three rooms just below the primary surface contain the secondary focus receivers, as well as smaller mirrors and electronics.
The telescope will ultimately have 0.3–115 GHz (1 metre to 3mm) continuous frequency coverage.
Initially three receivers were installed: an
L band receiver in prime focus, a
C-band receiver in the tertiary focus, and a 7-beam
K-band receiver in the secondary focus.
As of 2021, an upgrade was in progress to include two new receivers to cover more of the potential bandwith. This includes a set of 33-50 GHz receivers, and another set ranging from 70-116 GHz. This in turn requires the metrology and adjustment of the antenna be improved to allow efficient operation at such frequencies.
Collaboration, construction and commissioning
The telescope is a collaboration between several research units of the
National Institute for Astrophysics
The National Institute for Astrophysics (, or INAF) is an Italian research institute in astronomy and astrophysics, founded in 1999. INAF funds and operates twenty separate research facilities, which in turn employ scientists, engineers and techn ...
: the
Istituto di Radioastronomia di Bologna, the
Cagliari Observatory (Cagliari) and the
Arcetri Astrophysical Observatory. Construction was funded by the
Italian Ministry of Education and Scientific Research, the
Sardinia Regional Government, the
Italian Space Agency and INAF.
The telescope cost around €70 million to construct.
The contract to fabricate the telescope structure and mechanics started in 2003, and the construction of the foundations was completed in 2004. The initial schedule was for inauguration in late-2006;
construction ultimately was completed in mid-2012.
The telescope was constructed by MT Mechatronics GmbH of Germany. The
first light was on 8 August 2012, using the Moon and
3C218 (Alphard). The technical commissioning phase ended in 2013, and formal inauguration was on 30 September 2013,
with scientific commissioning between 2012 and 2015. Its first VLBI connection was in January 2014.
Science
The telescope can operate in single dish mode, measuring continuum, polarisation and spectra. It is also used for
very-long-baseline interferometry
Very-long-baseline interferometry (VLBI) is a type of astronomical interferometry used in radio astronomy. In VLBI a signal from an astronomical radio source, such as a quasar, is collected at multiple radio telescopes on Earth or in space. T ...
as part of the
European VLBI Network
The European VLBI Network (EVN) is a network of radio telescopes located primarily in Europe and Asia, with additional antennas in South Africa and Puerto Rico, which performs very high angular resolution observations of cosmic radio sources usin ...
, and with the space-based
RadioAstron antenna. It is also used for space science,
including deep space communication by the
Italian Space Agency.
References
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Radio telescopes
Sardinia