Pre-HEAT: submillimeter site testing and astronomical spectra from dome a, antarctica

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

doi:10.1117/12.789741

Pre-HEAT: submillimeter site testing and astronomical spectra from dome a, antarctica

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. YanJ. Yang, X. G. Zhang, X. Cui, X. Yuan, J. Hu, Z. Xu, Z. Jiang, H. Yang, Y. Li, B. Sun, W. Qin, Z. Shang

Research output: Chapter in Book/Report/Conference proceeding › Conference proceeding contribution › peer-review

20 Citations (Scopus)

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 ¹³CO 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.

Original language	English
Title of host publication	Ground-based and airborne telescopes II
Editors	Larry M. Stepp, Roberto Gilmozzi
Place of Publication	Bellingham, Washington
Publisher	SPIE
Pages	1-11
Number of pages	11
ISBN (Print)	9780819472229
DOIs	https://doi.org/10.1117/12.789741
Publication status	Published - 2008
Externally published	Yes
Event	Ground-based and Airborne Telescopes II - Marseille, France Duration: 23 Jun 2008 → 28 Jun 2008

Publication series

Name	Proceedings of SPIE
Publisher	SPIE
Number	7012
ISSN (Print)	0277-786X

Other

Other	Ground-based and Airborne Telescopes II
Country/Territory	France
City	Marseille
Period	23/06/08 → 28/06/08

Keywords

Antarctic astronomy
Heterodyne receiver
Interstellar medium
Site testing
Star formation
Submillimeter instrumentation
Terahertz spectroscopy

Access to Document

10.1117/12.789741

http://spiedl.aip.org/getabs/servlet/GetabsServlet?prog=normal&id=PSISDG007012000001701249000001&idtype=cvips&gifs=yes

Cite this

Kulesa, C. A., Walker, C. K., Schein, M., Golish, D., Tothill, N., Siegel, P., Weinreb, S., Jones, G., Bardin, J., Jacobs, K., Martin, C. L., Storey, J., Ashley, M., Lawrence, J., Luong-Van, D., Everett, J., Wang, L., Feng, L., Zhu, Z., ... Shang, Z. (2008). Pre-HEAT: submillimeter site testing and astronomical spectra from dome a, antarctica. In L. M. Stepp, & R. Gilmozzi (Eds.), Ground-based and airborne telescopes II (pp. 1-11). Article 701249 (Proceedings of SPIE; No. 7012). SPIE. https://doi.org/10.1117/12.789741

@inproceedings{0bc61bdd0a854beab397306ceebf7d21,

title = "Pre-HEAT: submillimeter site testing and astronomical spectra from dome a, antarctica",

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 13CO 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.",

keywords = "Antarctic astronomy, Heterodyne receiver, Interstellar medium, Site testing, Star formation, Submillimeter instrumentation, Terahertz spectroscopy",

author = "Kulesa, {C. A.} and Walker, {C. K.} and M. Schein and D. Golish and N. Tothill and P. Siegel and S. Weinreb and G. Jones and J. Bardin and K. Jacobs and Martin, {C. L.} and J. Storey and M. Ashley and J. Lawrence and D. Luong-Van and J. Everett and L. Wang and L. Feng and Z. Zhu and J. Yan and J. Yang and Zhang, {X. G.} and X. Cui and X. Yuan and J. Hu and Z. Xu and Z. Jiang and H. Yang and Y. Li and B. Sun and W. Qin and Z. Shang",

year = "2008",

doi = "10.1117/12.789741",

language = "English",

isbn = "9780819472229",

series = "Proceedings of SPIE",

publisher = "SPIE",

number = "7012",

pages = "1--11",

editor = "Stepp, {Larry M.} and Roberto Gilmozzi",

booktitle = "Ground-based and airborne telescopes II",

address = "United States",

note = "Ground-based and Airborne Telescopes II ; Conference date: 23-06-2008 Through 28-06-2008",

}

Kulesa, CA, Walker, CK, Schein, M, Golish, D, Tothill, N, Siegel, P, Weinreb, S, Jones, G, Bardin, J, Jacobs, K, Martin, CL, Storey, J, Ashley, M, Lawrence, J, Luong-Van, D, Everett, J, Wang, L, Feng, L, Zhu, Z, Yan, J, Yang, J, Zhang, XG, Cui, X, Yuan, X, Hu, J, Xu, Z, Jiang, Z, Yang, H, Li, Y, Sun, B, Qin, W & Shang, Z 2008, Pre-HEAT: submillimeter site testing and astronomical spectra from dome a, antarctica. in LM Stepp & R Gilmozzi (eds), Ground-based and airborne telescopes II., 701249, Proceedings of SPIE, no. 7012, SPIE, Bellingham, Washington, pp. 1-11, Ground-based and Airborne Telescopes II, Marseille, France, 23/06/08. https://doi.org/10.1117/12.789741

Pre-HEAT: submillimeter site testing and astronomical spectra from dome a, antarctica. / Kulesa, C. A.; Walker, C. K.; Schein, M. et al.
Ground-based and airborne telescopes II. ed. / Larry M. Stepp; Roberto Gilmozzi. Bellingham, Washington: SPIE, 2008. p. 1-11 701249 (Proceedings of SPIE; No. 7012).

Research output: Chapter in Book/Report/Conference proceeding › Conference proceeding contribution › peer-review

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AU - Kulesa, C. A.

AU - Walker, C. K.

AU - Schein, M.

AU - Golish, D.

AU - Tothill, N.

AU - Siegel, P.

AU - Weinreb, S.

AU - Jones, G.

AU - Bardin, J.

AU - Jacobs, K.

AU - Martin, C. L.

AU - Storey, J.

AU - Ashley, M.

AU - Lawrence, J.

AU - Luong-Van, D.

AU - Everett, J.

AU - Wang, L.

AU - Feng, L.

AU - Zhu, Z.

AU - Yan, J.

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AU - Zhang, X. G.

AU - Cui, X.

AU - Yuan, X.

AU - Hu, J.

AU - Xu, Z.

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AU - Li, Y.

AU - Sun, B.

AU - Qin, W.

AU - Shang, Z.

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N2 - 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 13CO 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.

AB - 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 13CO 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.

KW - Antarctic astronomy

KW - Heterodyne receiver

KW - Interstellar medium

KW - Site testing

KW - Star formation

KW - Submillimeter instrumentation

KW - Terahertz spectroscopy

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SN - 9780819472229

T3 - Proceedings of SPIE

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BT - Ground-based and airborne telescopes II

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PB - SPIE

CY - Bellingham, Washington

Y2 - 23 June 2008 through 28 June 2008

ER -

Pre-HEAT: submillimeter site testing and astronomical spectra from dome a, antarctica

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Keywords

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