The São Gião Radio Telescope is situated in the parish of São Gião Portugal. It was constructed in 2015, with first light in December 2015.[1] The gregorian telescope has a diameter of 9.3 m. As of 2019[update] it is the biggest radio telescope in mainland Portugal. Two 3 phase motors drive the azimuth and elevation (or altitude) servo systems with an accuracy of 0.01 degree. The main reflector has a solid reflector surface that makes it suitable for observations of high frequencies up to 22 GHz.
![]() São Gião Radio Telescope | |
Location(s) | São Gião, Oliveira do Hospital, Coimbra District, Portugal |
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Coordinates | 40°19′49″N 7°48′47″W ![]() |
Altitude | 704 m (2,310 ft) ![]() |
Telescope style | radio telescope ![]() |
Diameter | 9.3 m (30 ft 6 in) ![]() |
Website | www![]() |
![]() ![]() Location of São Gião Radio Telescope | |
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It is used to observe the hydrogen line from our galaxy and maser signals from star-forming regions and late evolution AGB or OH/IR stars.[2] The frequencies used for the hydrogen line is 1.42 GHz and maser signals are measured on 1.612,[3] and 12 GHz[4] The data results obtained with the telescope were presented on EUCARA 2016 Dwingeloo Netherlands [5] and on the ASTROFESTA 2018 in Constancia Portugal.[6][7] The telescope data and methods are also referenced by universities like the Western Kentucky University,[8] and societies like Ofiuco[9] and the Society of Amateur Radio Astronomers.[10]
A report from the Correio da Beira Serra newspaper about the São Gião radio telescope, can be consulted here.