385:, claimed that the bi-national agreement did not provide for the creation of a separate observatory. They argued that the telescope should ultimately be under the control of the Director of Mount Stromlo and Siding Spring Observatories and that additional staff for the new telescope should be provided by the ANU. However, fearing that they would be mere guests rather than equal partners in the AAT, British astronomers, with support from Australian state university astronomers, campaigned hard for a separate director and staff who were employed by and answerable only to the AATB. The matter was not settled until June 1973 when the Australian government endorsed the AATBs decision for an independent staff, marking the birth of the Anglo-Australian Observatory. The first director, Joe Wampler, took up his post in September 1974. To date there have been five directors.
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respectively, began in late-1970 and was completed by the end of 1972. The building was manufactured from concrete, stands 26m high and has seven floors housing offices, labs and a mirror aluminising chamber. The telescope stands on a concrete pier with a separate foundation to the main building, to
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After a series of meetings between
British and Australian scientists in the early 1960s to discuss the technical specifications and begin the search for a suitable site for the proposed telescope, a formal approach was made to the governments of both countries in July 1965. It was finally agreed in
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for ~250000 galaxies brighter than B~19.5 over ~7% of the southern sky in only ~270 nights. The 2dFGRS sample size was an order of magnitude greater than those of previous surveys, allowing a rigorous evaluation of cosmological parameters. For example, the survey has refined estimates of the mass
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is using the AAT and AAOmega to measure the redshifts of ~200000 distant luminous blue star forming galaxies distributed over an area of ~5000 times the area of the moon. The primary goal of this study is to use an intrinsic feature in the distribution of galaxies as a "standard ruler" to relate
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The Anglo-Australian
Telescope Agreement was signed on 25 September 1969 and came into effect on 22 February 1971. The Joint Policy Committee was replaced by the Anglo-Australian Telescope Board (AATB), an entity with full legal status under Australian law with responsibilities of overseeing the
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where it is dispersed into its component colours for detailed subsequent analysis. The broad field-of-view accessed by the 2dF and AAOmega instruments (4 times the width of the moon) and their 400 optical fibres, makes it feasible to spectroscopically survey large numbers of objects distributed
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was built to complement the AAT and officially began operations in August 1973. It was designed for survey astronomy, having an extremely large field-of-view which is more than 12 times the apparent diameter of the moon. The telescope was operated by the
Schmidt Telescope Unit of the
444:. It was shipped to Australia in early 1973 before being assembled at Siding Spring Mountain in April of that year. The telescope drive system was also produced by Mitsubishi Electric and delivered at this time. It was one of the first to be controlled by computer, an
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Model 70, and provided new levels of pointing and tracking precision. Assembly of the AAT was completed by 1974 and commissioning of the telescope began in April of that year. In total it took eight years to build at a cost of A$ 16 million. It was inaugurated by
365:. The project office finalised designs and specifications for the telescope, the mounting and the building and let contracts on a worldwide basis, exploiting the experience of those staff members who were involved in the development and construction of the
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521:(AAPS). The AAPS exploits the high stability of the University College London Echelle Spectrograph (UCLES) to obtain the few metres per second precision in measurements of the line-of-sight velocities of stars necessary to detect the reflex
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The
Australian Astronomical Observatory in 2008 (then called the "Anglo-Australian Observatory"). The staff tea room is in the lower left corner and the workshop to the right. The kangaroos in the foreground are a common sight at
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matter in the
Universe and set an upper limit on the total mass of neutrinos. In addition 2dFGRS yielded an independent estimate of the Hubble constant, which was in excellent agreement with value determined by the
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As construction of the AAT gathered pace, a heated debate ensued as to the details of the management structure which would control the telescope. Then
Director of Mount Stromlo and Siding Spring Observatories,
506:(GAMA), is in the process of obtaining optical spectroscopy for ~250000 galaxies in the Local Universe. The AAOmega data will be used in conjunction with observations from satellite observatories such as the
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In addition to operating the two telescopes, AAO staff carried out astronomical research, and designed and built astronomical instrumentation for the AAT, UKST, and other telescopes including the
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distance to redshift and improve our knowledge of the nature of dark energy. This mysterious component of the
Universe appears to be responsible for accelerating its rate of expansion.
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in astronomy for over 25 years. Instruments such as AAOmega, and its predecessor 2dF, use optical fibres to feed the light of stars and galaxies from the telescope into a
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governments, it was managed wholly by
Australia's Department of Industry, Innovation, Science, Research and Tertiary Education. The AAO operated the 3.9-metre
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induced by the presence of a planet. The AAPS has found more than 20 extrasolar planets, with masses ranging from ~10% to > 10 times that of
Jupiter.
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optical observational astronomy in the UK was toiling due to a lack of modern infrastructure. There were no large telescopes in the
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reduce the risk of vibrations. The double skinned dome is manufactured from both steel and aluminium and weighs 570 tonnes.
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361:(UK) and Jim Hosie (UK) was formed to oversee the early running of a project office which was located in
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The
Schmidt has undertaken work including blue and red photographic surveys of the southern sky and the
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Later that year an interim body known as the Joint Policy Committee, and including prominent scientists
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Anglo-Australian Observatory Observers Guide. eds. E. Sadler, S. Harrison and S. Lee, AAO UM1.4
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A number of major studies undertaken with the AAT have exploited these capabilities. The
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International Convention for the Suppression of the Traffic in Women and Children
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Construction of the building and dome, undertaken by the Australian companies
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until 1988, when it was agreed that control would be handed over to the AAO.
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from 1956 to 1971, suggested constructing a large telescope in Australia.
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Declaration recognising the Right to a Flag of States having no Sea-coast
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Agreement for the Suppression of the Circulation of Obscene Publications
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International Agreement for the suppression of the White Slave Traffic
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The final product has a diameter of 3.9m and a focal length of 12.7m.
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In late-1967 the contract for the primary mirror blank was awarded to
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density of the Universe, provided a determination of the fraction of
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603:(press release), Australian Astronomical Observatory, archived from
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despite some of the most intriguing astronomical objects (e.g. the
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314:) being best placed for study from these latitudes. In the 1950s
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on 16 October 1974 and went into general use in June 1975.
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Paris Convention for the Protection of Industrial Property
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across expansive areas of sky in a reasonable time frame.
334:(AAT), should proceed. The telescope was to be located on
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British Army regiments in Australia between 1810 and 1870
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Second Australian Imperial Force in the United Kingdom
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April 1967 that the building of a 150" telescope, the
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Australian Constitution (Public Record Copy) Act 1990
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High Commissioners of the United Kingdom to Australia
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High Commissioners of Australia to the United Kingdom
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Blake, C. and the WiggleZ team, 2008, A&G, 49, 19
833:". 1 April 2009, Australian Astronomical Observatory
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844:"RAVE webpages at Astrophysics Institute Potsdam"
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695:The Creation of the Anglo-Australian Observatory
193:Location of Australian Astronomical Observatory
726:. Aao.gov.au. 16 November 2012. Archived from
401:glass in April 1969. The blank was shipped to
389:Construction of the Anglo-Australian Telescope
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1011:2011 Commonwealth Heads of Government Meeting
1006:2002 Commonwealth Heads of Government Meeting
1001:1981 Commonwealth Heads of Government Meeting
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405:, England to be figured and polished by
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1016:Judicial Committee of the Privy Council
640:"UK pulls funding from joint telescope"
600:The Anglo-Australian Telescope turns 35
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381:and then Vice-Chancellor of the ANU,
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955:High Commission of Australia, London
846:. Rave-survey.aip.de. Archived from
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872:Australian Astronomical Observatory
235:. Originally funded jointly by the
217:Australian Astronomical Observatory
22:Australian Astronomical Observatory
1266:British nuclear tests at Maralinga
1094:Southeast Asia Treaty Organization
934:Australia–United Kingdom relations
792:Galaxy and Mass Assembly web pages
597:Helen Sim, ed. (14 October 2009),
574:List of astronomical observatories
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1152:Australian Constitutions Act 1850
965:British High Commission, Canberra
755:". Australian National University
751:" Colless, Matthew (5 July 2012)
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1089:Five Power Defence Arrangements
298:In the years immediately after
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753:The 2dF Galaxy Redshift Survey
519:Anglo-Australian Planet Search
430:Kitt Peak National Observatory
344:Australian National University
1:
796:European Southern Observatory
646:. Abc.net.au. 15 October 2009
264:European Southern Observatory
110:1,164 m (3,819 ft)
798:, Retrieved 15 January 2013.
546:Royal Observatory, Edinburgh
91:33.79621012°S 151.14511752°E
1286:McClelland Royal Commission
1162:Statute of Westminster 1931
831:6dF Galaxy Survey web pages
772:, Retrieved 15 January 2013
666:"Leighton Holdings History"
270:in Chile, and the Japanese
255:, located near the town of
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1312:Anglo-Australian Telescope
1111:RAAF Overseas Headquarters
882:2dF Quasar Redshift Survey
877:2dF Galaxy Redshift Survey
557:Radial Velocity Experiment
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508:Herschel Space Observatory
475:2dF Galaxy Redshift Survey
373:running of the telescope.
332:Anglo-Australian Telescope
245:Anglo-Australian Telescope
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96:-33.79621012; 151.14511752
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1334:Britain–Australia Society
1099:British Army in Australia
724:"AAOmega web page at AAO"
424:The telescope is mounted
342:, which was owned by the
320:Mount Stromlo Observatory
253:Siding Spring Observatory
223:with its headquarters in
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1147:South Australia Act 1842
1142:South Australia Act 1834
1137:New South Wales Act 1823
1023:Royal tours of Australia
887:27 February 2021 at the
809:"AAPS web pages at UNSW"
504:Galaxy and Mass Assembly
461:The AAO has made use of
1203:Berne Convention (1906)
996:Commonwealth of Nations
418:Evans-Deakin Industries
1372:The Queen in Australia
1319:Australian State Coach
991:Nauru Island Agreement
489:Hubble Space Telescope
367:Parkes radio telescope
336:Siding Spring Mountain
322:from 1939 to 1956 and
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36:Alternative names
1365:A Bride from the Bush
1349:Monarchy of Australia
529:The Schmidt Telescope
457:Research with the AAT
292:
1329:Big Brother Movement
770:Swinburne University
569:Digitized Sky Survey
541:UK Schmidt Telescope
535:UK Schmidt Telescope
414:Leighton Contractors
268:Very Large Telescope
249:UK Schmidt Telescope
247:(AAT) and 1.2-metre
155:UK Schmidt Telescope
1276:Operation Hurricane
676:on 11 December 2007
442:Mitsubishi Electric
403:Newcastle-upon-Tyne
304:southern hemisphere
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1271:Operation Blowdown
1172:Australia Act 1986
1055:Military relations
811:. Phys.unsw.edu.au
515:extrasolar planets
451:HRH Prince Charles
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850:on 20 August 2009
730:on 5 January 2013
670:Leighton Holdings
628:. 4 January 2018.
607:on 5 January 2013
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