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Pre-HEAT: submillimeter site testing and astronomical spectra from Dome A, Antarctica

Kulesa, C. A. and Walker, C. K. and Schein, M. and Golish, D. and Tothill, N. and Siegel, P. and Weinreb, S. and Jones, G. and Bardin, J. and Jacobs, K. and Martin, C. L. and Storey, J. and Ashley, M. and Lawrence, J. and Luong-Van, D. and Everett, J. and Wang, L. and Feng, L. and Zhu, Z. and Yan, J. and Yang, J. and Zhang, X.-G. and Cui, X. and Yuan, X. and Hu, J. and Xu, Z. and Jiang, Z. and Yang, H. and Li, Y. and Sun, B. and Qin, W. and Shang, Z. (2008) Pre-HEAT: submillimeter site testing and astronomical spectra from Dome A, Antarctica. In: Ground-based and Airborne Telescopes II. Proceedings of SPIE. No.7012. Society of Photo-optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. no. 701249. ISBN 9780819472229. https://resolver.caltech.edu/CaltechAUTHORS:20180802-154730971

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Abstract

Pre-HEAT is a 20 cm aperture submillimeter-wave telescope with a 660 GHz (450 micron) Schottky diode heterodyne receiver and digital FFT spectrometer for the Plateau Observatory (PLATO) developed by the University of New South Wales. In January 2008 it was deployed to Dome A, the summit of the Antarctic plateau, as part of a scientific traverse led by the Polar Research Institute of China and the Chinese Academy of Sciences. Dome A may be one of the best sites in the world for ground based Terahertz astronomy, based on the exceptionally cold, dry and stable conditions which prevail there. Pre-HEAT is measuring the 450 micron sky opacity at Dome A and mapping the Galactic Plane in the ^(13)CO J=6-5 line, constituting the first submillimeter measurements from Dome A. It is field-testing many of the key technologies for its namesake -- a successor mission called HEAT: the High Elevation Antarctic Terahertz telescope. Exciting prospects for submillimeter astronomy from Dome A and the status of Pre-HEAT will be presented.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1117/12.789741DOIArticle
ORCID:
AuthorORCID
Siegel, P.0000-0002-2539-4646
Wang, L.0000-0002-9803-166X
Additional Information:© 2008 Society of Photo-Optical Instrumentation Engineers (SPIE). The authors wish to thank all members of the Polar Research Institute of China's 2008 Dome A expedition for their heroic efforts in reaching the summit and for providing invaluable assistance to the expedition astronomers in setting up the PLATO observatory and its attendant instruments. Construction of Pre-HEAT was financially supported from the US National Science Foundation under the auspices of Small Grants for Exploratory Research (ANT-0735854).
Funders:
Funding AgencyGrant Number
NSFANT-0735854
Subject Keywords:site testing, Antarctic astronomy, submillimeter instrumentation, terahertz spectroscopy, heterodyne receiver, interstellar medium, star formation
Series Name:Proceedings of SPIE
Issue or Number:7012
Record Number:CaltechAUTHORS:20180802-154730971
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20180802-154730971
Official Citation:C. A. Kulesa, C. K. Walker, M. Schein, D. Golish, N. Tothill, P. Siegel, S. Weinreb, G. Jones, J. Bardin, K. Jacobs, C. L. Martin, J. Storey, M. Ashley, J. Lawrence, D. Luong-Van, J. Everett, L. Wang, L. Feng, Z. Zhu, J. Yan, J. Yang, X.-G. Zhang, X. Cui, X. Yuan, J. Hu, Z. Xu, Z. Jiang, H. Yang, Y. Li, B. Sun, W. Qin, Z. Shang, "Pre-HEAT: submillimeter site testing and astronomical spectra from Dome A, Antarctica", Proc. SPIE 7012, Ground-based and Airborne Telescopes II, 701249 (10 July 2008); doi: 10.1117/12.789741; https://doi.org/10.1117/12.789741
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:88542
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:03 Aug 2018 20:42
Last Modified:10 Mar 2020 18:21

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