Li, Yushan Zheng, Jessica Tuthill, Peter Freeman, Matthew Ashley, Michael Burton, Michael Lawrence, Jon Mould, Jeremy and Wang, Lifan 2016. Optimising the K Dark Filter for the Kunlun Infrared Sky Survey. Publications of the Astronomical Society of Australia, Vol. 33,
Fruth, T. Cabrera, J. Csizmadia, Sz. Dreyer, C. Eigmüller, P. Erikson, A. Kabath, P. Pasternacki, T. Rauer, H. Titz-Weider, R. Abe, L. Agabi, A. Gonçalves, I. Guillot, T. Mékarnia, D. Rivet, J.-P. Crouzet, N. Chini, R. Lemke, R. and Murphy, M. 2014. Transit Search from Antarctica and Chile—Comparison and Combination. Publications of the Astronomical Society of the Pacific, Vol. 126, Issue. 937, p. 227.
Bond, Ian A. 2012. The first extrasolar planet detected via gravitational microlensing. New Astronomy Reviews, Vol. 56, Issue. 1, p. 25.
Mould, Jeremy 2012. Next Generation Deep 2μm Survey. Proceedings of the International Astronomical Union, Vol. 8, Issue. S288, p. 239.
Storey, John W. V. Abe, Lyu Andersen, Michael Anderson, Philip Burton, Michael Cui, Xiangqun Ichikawa, Takashi Karle, Albrecht Lloyd, James Masi, Silvia Steinbring, Eric Travouillon, Tony Tuthill, Peter and Zhou, HongYang 2012. The SCAR Astronomy & Astrophysics from Antarctica Scientific Research Programme. Proceedings of the International Astronomical Union, Vol. 8, Issue. S288, p. 275.
Burton, Michael G. 2010. Astronomy in Antarctica. The Astronomy and Astrophysics Review, Vol. 18, Issue. 4, p. 417.
Di Rico, Gianluca Ragni, Maurizio Dolci, Mauro Straniero, Oscar Valentini, Angelo Valentini, Gaetano Di Cianno, Amico Giuliani, Croce Magrin, Demetrio Bonoli, Carlotta Bortoletto, Favio D'Alessandro, Maurizio Corcione, Leonardo and Riva, Alberto 2010. Autonomous Observations in Antarctica with AMICA. Advances in Astronomy, Vol. 2010, p. 1.
Zou, Hu Zhou, Xu Jiang, Zhaoji Ashley, M. C. B. Cui, Xiangqun Feng, Longlong Gong, Xuefei Hu, Jingyao Kulesa, C. A. Lawrence, J. S. Liu, Genrong Luong-Van, D. M. Ma, Jun Moore, A. M. Pennypacker, C. R. Qin, Weijia Shang, Zhaohui Storey, J. W. V. Sun, Bo Travouillon, T. Walker, C. K. Wang, Jiali Wang, Lifan Wu, Jianghua Wu, Zhenyu Xia, Lirong Yan, Jun Yang, Ji Yang, Huigen Yao, Yongqiang Yuan, Xiangyan York, D. G. Zhang, Zhanhai and Zhu, Zhenxi 2010. SKY BRIGHTNESS AND TRANSPARENCY IN THEi-BAND AT DOME A, ANTARCTICA. The Astronomical Journal, Vol. 140, Issue. 2, p. 602.
Lawrence, J. S. Ashley, M. C. B. Hengst, S. Luong-Van, D. M. Storey, J. W. V. Yang, H. Zhou, X. and Zhu, Z. 2009. The PLATO Dome A site-testing observatory: Power generation and control systems. Review of Scientific Instruments, Vol. 80, Issue. 6, p. 064501.
Zinnecker, Hans 2009. Astronomy from the Antarctic Plateau: a global personal vision. Proceedings of the International Astronomical Union, Vol. 5, Issue. H15, p. 636.
Ellis, S. C. and Bland-Hawthorn, J. 2008. The case for OH suppression at near-infrared wavelengths. Monthly Notices of the Royal Astronomical Society, Vol. 386, Issue. 1, p. 47.
Kankare, E. Mattila, S. Ryder, S. Pérez-Torres, M.-A. Alberdi, A. Romero-Canizales, C. Díaz-Santos, T. Väisänen, P. Efstathiou, A. Alonso-Herrero, A. Colina, L. and Kotilainen, J. 2008. Discovery of a Very Highly Extinguished Supernova in a Luminous Infrared Galaxy. The Astrophysical Journal, Vol. 689, Issue. 2, p. L97.
Lawrence, J. S. Ashley, M. C. B. Storey, J. W. V. Jolissaint, L. and Travouillon, T. 2008. Adaptive Optics Sky Coverage for Dome C Telescopes. Publications of the Astronomical Society of the Pacific, Vol. 120, Issue. 872, p. 1119.
Di Rico, Gianluca 2007. An Automatic Control System for Acquisition and Processing of Infrared Data in the Antarctic Environment. Publications of the Astronomical Society of the Pacific, Vol. 119, Issue. 860, p. 1206.
Strassmeier, K. G. Agabi, K. Agnoletto, L. Allan, A. Andersen, M. I. Ansorge, W. Bortoletto, F. Briguglio, R. Buey, J.-T. Castellini, S. Coudé du Foresto, V. Damé, L. Deeg, H. J. Eiroa, C. Durand, G. Fappani, D. Frezzotti, M. Granzer, T. Gröschke, A. Kärcher, H. J. Lenzen, R. Mancini, A. Montanari, C. Mora, A. Pierre, A. Pirnay, O. Roncella, F. Schmider, F.-X. Steele, I. Storey, J. W. V. Tothill, N. F. H. Travouillon, T. Vittuari, L. and Weber, M. 2007. Telescope and instrument robotization at Dome C. Astronomische Nachrichten, Vol. 328, Issue. 6, p. 451.
Bland-Hawthorn, J. 2006. Stellar populations – the next ten years. Proceedings of the International Astronomical Union, Vol. 2, Issue. S241,
Burton, Michael G. 2006. Special Session 7 Astronomy in Antartica. Proceedings of the International Astronomical Union, Vol. 2, Issue. 14,
Kelz, Andreas 2006. Antarctica – a case for 3D-spectroscopy. Proceedings of the International Astronomical Union, Vol. 2, Issue. 14,
Kenyon, S. L. and Storey, J. W. V. 2006. A Review of Optical Sky Brightness and Extinction at Dome C, Antarctica. Publications of the Astronomical Society of the Pacific, Vol. 118, Issue. 841, p. 489.
Riva, Alberto Dolci, Mauro Straniero, Oscar Zerbi, Filippo Maria Molinari, Emilio Conconi, Paolo De Caprio, Vincenzo Valentini, Gaetano Di Rico, Gianluca Ragni, Maurizio Pelusi, Danilo Di Varano, Igor Giuliani, Croce Di Cianno, Amico Valentini, Angelo Bortoletto, Favio D'Alessandro, Maurizio Bonoli, Carlotta Giro, Enrico Fantinel, Daniela Magrin, Demetrio Corcione, Leonardo Busso, Maurizio Tosti, Gino Nucciarelli, Giuliano Roncella, Fabio and Abia, Carlos 2006. AMICA – the infrared eye at Dome C. Proceedings of the International Astronomical Union, Vol. 2, Issue. 14,
The cold, dry, and stable air above the summits of the Antarctic plateau provides the best ground-based observing conditions from optical to sub-millimetre wavelengths to be found on the Earth. Pathfinder for an International Large Optical Telescope (PILOT) is a proposed 2 m telescope, to be built at Dome C in Antarctica, able to exploit these conditions for conducting astronomy at optical and infrared wavelengths. While PILOT is intended as a pathfinder towards the construction of future grand-design facilities, it will also be able to undertake a range of fundamental science investigations in its own right. This paper provides the performance specifications for PILOT, including its instrumentation. It then describes the kinds of projects that it could best conduct. These range from planetary science to the search for other solar systems, from star formation within the Galaxy to the star formation history of the Universe, and from gravitational lensing caused by exo-planets to that produced by the cosmic web of dark matter. PILOT would be particularly powerful for wide-field imaging at infrared wavelengths, achieving near diffraction-limited performance with simple tip–tilt wavefront correction. PILOT would also be capable of near diffraction-limited performance in the optical wavebands, as well be able to open new wavebands for regular ground-based observation, in the mid-IR from 17 to 40 μm and in the sub-millimetre at 200 μm.
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