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Dome C site testing: implications for science and technology of future telescopes Proceedings of the 3rd ARENA Conference, EAS Publications Series, 2010 (Ref: 14029)
Category 3: Conference paper

Site testing data provides an essential part of the justi¯cation … for funding any new astronomical facility by de¯ning the technological … design and determining the telescope performance, thus allowing the … scienti¯c objectives to be prioritised.

A wide-field, optical/infrared, 2.5m class telescope for Antarctica Proceedings of the 3rd ARENA Conference, EAS Publications Series, 2010 (Ref: 14022)
Category 3: Conference paper

This report provides the recommendations of ARENAWork- … ing Group 1 concerning the development of and objectives for a wide- … field, optical / infrared, 2.5m class telescope for Antarctica. It discusses … the key science drivers for such a telescope…

The Science Case for PILOT II: the Distant Universe Publications of the Astronomical Society of Australia, 2009 (Ref: 14014)
Category 1: Peer-reviewed literature

PILOT (the Pathfinder for an International Large Optical Telescope) is a proposed 2.5-m optical/ … infrared telescope to be located at Dome C on the Antarctic plateau. The atmospheric conditions at Dome C … deliver a high sensitivity, high photometric precision, wide-field, high spatial resolution…

The Science Case for PILOT III: the Nearby Universe Publications of the Astronomical Society of Australia, 2009 (Ref: 14013)
Category 1: Peer-reviewed literature

PILOT (the Pathfinder for an International Large Optical Telescope) is a proposed 2.5-m optical/ … infrared telescope to be located at Dome C on the Antarctic plateau. The atmospheric conditions at Dome C … deliver a high sensitivity, high photometric precision, wide-field, high spatial resolution…

Proposed intrumentation for PILOT Proceedings of SPIE 7014, 70144N1-9, 2008 (Ref: 13757)
Category 3: Conference paper

PILOT (the Pathfinder for an International Large Optical Telescope) is a proposed Australian/European optical/infrared … telescope for Dome C on the Antarctic Plateau, with target first light in 2012. The proposed telescope is 2.4m diameter, with overall focal ratio f/10…

Twilight astronomy from Antarctica Proceedings of the 2nd ARENA Conference, EAS Publications Series, 2008 (Ref: 13761)
Authors:
Category 3: Conference paper

A description of the early days of infrared site testing at … the South Pole is given, with special attention paid to the data which … quantified the conditions during summer and the long twilight period. Such times are also provide relatively benign conditions for humans … in Antarctica as well.

PILOT-like telescope potential Proceedings of the 2nd ARENA Conference, EAS Publications Series, 2008 (Ref: 13758)
Category 3: Conference paper

In this paper we review the progress towards the deployment … of a large "PILOT-like" telescope at Concordia Station, Dome C. PI- … LOT is a proposed 2.4m optical/IR telescope that will cost in excess … of EUR 10m…

Mark recapture analysis of Pygmy Blue Whales from Perth Canyon, Western Australia 2000-2005 IWC Scientific Committee; SC/60/SH16, 2008 (Ref: 13451)
Category 2: International meeting papers

Between January and April over six consecutive years (2000 to 2005) photographs of the … dorsal fin and lateral bodies of pygmy blue whales (Balaenoptera musculus brevicauda) were … collected at the Perth Canyon, Western Australia.

LAPCAT: the Large Antarctic Plateau Clear-Aperture Telescope Ground-based and Airborne Telescopes, Proceedings of the SPIE, 2006 (Ref: 12901)
Category 3: Conference paper

We present a proposal for an 8.4 metre off-axis optical/IR telescope to be located at Dome C, Antarctica. LAPCAT will use a mirror identical to the offset segment recently cast for the Giant Magellan Telescope (GMT) as a completely unobscured f/2.1 primary.

Site testing Dome A, Antarctica Ground-based and Airborne Telescopes, Proceedings of the SPIE, 2006 (Ref: 12899)
Category 3: Conference paper

Recent data have shown that Dome C, on the Antarctic plateau, is an exceptional site for astronomy, with atmospheric conditions superior to those at any existing mid-latitude site. Dome C, however, may not be the best site on the Antarctic plateau for every kind of astronomy.

Exoplanet detection from Dome C, Antarctica: opportunities and challenges IAU Colloquium 200, Direct Imaging of Exoplanets: Science and Techniques, Nice, France, 2006 (Ref: 12895)
Category 3: Conference paper

Many methods have been proposed for the detection of exoplanets. The minimum … detectable planetary size and mass, and the maximum distance from us at which exoplanets are … observable, are determined by both technological and environmental constraints.

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