Sardinia Radio Telescope
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The Sardinia Radio Telescope (SRT) is 64-metre fully steerable radio telescope near San Basilio,
Province of Cagliari Cagliari ( it, provincia di Cagliari; sc, provìntzia de Casteddu) was a province in the autonomous island region of Sardinia, Italy and its capital city was Cagliari. It had an area of , and a total population of 543,310 (2001). There were 71 ...
,
Sardinia Sardinia ( ; it, Sardegna, label=Italian, Corsican and Tabarchino ; sc, Sardigna , sdc, Sardhigna; french: Sardaigne; sdn, Saldigna; ca, Sardenya, label= Algherese and Catalan) is the second-largest island in the Mediterranean Sea, aft ...
, Italy. Completed in 2011, it is a collaboration between the Istituto di Radioastronomia di Bologna, the
Cagliari Observatory The Cagliari Observatory ( it, Osservatorio Astronomico di Cagliari, or OAC) is an astronomical observatory owned and operated by Italy's Istituto Nazionale di Astrofisica (National Institute for Astrophysics, INAF). It is located 20 km away ...
(Cagliari) and the Arcetri Astrophysical Observatory (Florence).


Design

The telescope is in Sardinia, north of
Cagliari Cagliari (, also , , ; sc, Casteddu ; lat, Caralis) is an Italian municipality and the capital of the island of Sardinia, an autonomous region of Italy. Cagliari's Sardinian name ''Casteddu'' means ''castle''. It has about 155,000 inhabitant ...
, and is the largest of a set of three telescopes operated by
INAF The National Institute for Astrophysics ( it, Istituto Nazionale di Astrofisica, 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 e ...
, along with telescopes at the
Medicina Radio Observatory The Medicina Radio Observatory is an astronomical observatory located 30 km from Bologna, Italy. It is operated by the Institute for Radio Astronomy of the National Institute for Astrophysics (INAF) of the government of Italy. The site incl ...
and the
Noto Radio Observatory The Noto VLBI Station is a radio observatory located on Sicily, southern Italy, outside the city of Noto. The facility is operated by the Istituto di Radioastronomia di Bologna. The antenna is a 32-metre diameter paraboloid fitted with an activ ...
. 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 An active surface is a surface of a radio telescope that is under active computer control of its shape. Large (more than 10 m in diameter or length) radio telescopes always bend during operation, due to their enormous weight and the fact tha ...
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 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 triangulate a scale map on sit ...
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 The L band is the Institute of Electrical and Electronics Engineers (IEEE) designation for the range of frequencies in the radio spectrum from 1 to 2 gigahertz (GHz). This is at the top end of the ultra high frequency (UHF) band, at the lower en ...
receiver in prime focus, a C-band receiver in the tertiary focus, and a 7-beam K-band receiver in the secondary focus.


Collaboration, construction and commissioning

The telescope is a collaboration between the research units of the
National Institute for Astrophysics The National Institute for Astrophysics ( it, Istituto Nazionale di Astrofisica, 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 e ...
: the Istituto di Radioastronomia di Bologna, the
Cagliari Observatory The Cagliari Observatory ( it, Osservatorio Astronomico di Cagliari, or OAC) is an astronomical observatory owned and operated by Italy's Istituto Nazionale di Astrofisica (National Institute for Astrophysics, INAF). It is located 20 km away ...
(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 The Italian Space Agency ( it, Agenzia Spaziale Italiana; ASI) is a government agency established in 1988 to fund, regulate and coordinate space exploration activities in Italy. The agency cooperates with numerous national and international enti ...
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. Th ...
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 The Italian Space Agency ( it, Agenzia Spaziale Italiana; ASI) is a government agency established in 1988 to fund, regulate and coordinate space exploration activities in Italy. The agency cooperates with numerous national and international enti ...
.


References

{{authority control Radio telescopes Sardinia