Abstract
![CDATA[The South Pole Imaging Fabry-Perot Interferometer, SPIFI, is a direct detection imaging spectrometer for submillimeter astronomy in the telluric windows at 200 pm, 350 m, and 450 pm that are available at the South Pole (B1, B2). The main components of SPIFI are the cryogenic Fabry-Perot interferometers (FPI's) which can be tuned to any wavelength within the atmospheric windows and the detector array which provides a two dimensional field of view.]]
| Original language | English |
|---|---|
| Title of host publication | Proceedings of the 15th International Symposium on Space Terahertz Technology, April 27-29, 2004, Hotel Northampton, Northampton, Massachusetts |
| Publisher | National Radio Astronomy Observatory |
| Pages | 357-364 |
| Number of pages | 8 |
| Publication status | Published - 2004 |
| Event | International Symposium on Space Terahertz Technology - Duration: 1 Jan 2008 → … |
Conference
| Conference | International Symposium on Space Terahertz Technology |
|---|---|
| Period | 1/01/08 → … |
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Nikola, T., Stacey, G. J., Oberst, T. E., Parshley, S. C., Stark, A. A., Tothill, N., & Harnett, J. (2004). SPIFI : The South Pole Imaging Fabry-Perot Interferometer on AST/RO. In Proceedings of the 15th International Symposium on Space Terahertz Technology, April 27-29, 2004, Hotel Northampton, Northampton, Massachusetts (pp. 357-364). National Radio Astronomy Observatory.
Nikola, T. ; Stacey, G. J. ; Oberst, T. E. et al. / SPIFI : The South Pole Imaging Fabry-Perot Interferometer on AST/RO. Proceedings of the 15th International Symposium on Space Terahertz Technology, April 27-29, 2004, Hotel Northampton, Northampton, Massachusetts. National Radio Astronomy Observatory, 2004. pp. 357-364
@inproceedings{5acaf1b2dc7047739ae9bb6412636af1,
title = "SPIFI : The South Pole Imaging Fabry-Perot Interferometer on AST/RO",
abstract = "![CDATA[The South Pole Imaging Fabry-Perot Interferometer, SPIFI, is a direct detection imaging spectrometer for submillimeter astronomy in the telluric windows at 200 pm, 350 m, and 450 pm that are available at the South Pole (B1, B2). The main components of SPIFI are the cryogenic Fabry-Perot interferometers (FPI's) which can be tuned to any wavelength within the atmospheric windows and the detector array which provides a two dimensional field of view.]]",
author = "T. Nikola and Stacey, {G. J.} and Oberst, {T. E.} and Parshley, {S. C.} and Stark, {A. A.} and N. Tothill and J. Harnett",
year = "2004",
language = "English",
pages = "357--364",
booktitle = "Proceedings of the 15th International Symposium on Space Terahertz Technology, April 27-29, 2004, Hotel Northampton, Northampton, Massachusetts",
publisher = "National Radio Astronomy Observatory",
note = "International Symposium on Space Terahertz Technology ; Conference date: 01-01-2008",
}
Nikola, T, Stacey, GJ, Oberst, TE, Parshley, SC, Stark, AA, Tothill, N & Harnett, J 2004, SPIFI : The South Pole Imaging Fabry-Perot Interferometer on AST/RO. in Proceedings of the 15th International Symposium on Space Terahertz Technology, April 27-29, 2004, Hotel Northampton, Northampton, Massachusetts. National Radio Astronomy Observatory, pp. 357-364, International Symposium on Space Terahertz Technology, 1/01/08.
SPIFI : The South Pole Imaging Fabry-Perot Interferometer on AST/RO. / Nikola, T.; Stacey, G. J.; Oberst, T. E. et al.
Proceedings of the 15th International Symposium on Space Terahertz Technology, April 27-29, 2004, Hotel Northampton, Northampton, Massachusetts. National Radio Astronomy Observatory, 2004. p. 357-364.
Research output: Chapter in Book / Conference Paper › Conference Paper
TY - GEN
T1 - SPIFI : The South Pole Imaging Fabry-Perot Interferometer on AST/RO
AU - Nikola, T.
AU - Stacey, G. J.
AU - Oberst, T. E.
AU - Parshley, S. C.
AU - Stark, A. A.
AU - Tothill, N.
AU - Harnett, J.
PY - 2004
Y1 - 2004
N2 - ![CDATA[The South Pole Imaging Fabry-Perot Interferometer, SPIFI, is a direct detection imaging spectrometer for submillimeter astronomy in the telluric windows at 200 pm, 350 m, and 450 pm that are available at the South Pole (B1, B2). The main components of SPIFI are the cryogenic Fabry-Perot interferometers (FPI's) which can be tuned to any wavelength within the atmospheric windows and the detector array which provides a two dimensional field of view.]]
AB - ![CDATA[The South Pole Imaging Fabry-Perot Interferometer, SPIFI, is a direct detection imaging spectrometer for submillimeter astronomy in the telluric windows at 200 pm, 350 m, and 450 pm that are available at the South Pole (B1, B2). The main components of SPIFI are the cryogenic Fabry-Perot interferometers (FPI's) which can be tuned to any wavelength within the atmospheric windows and the detector array which provides a two dimensional field of view.]]
UR - http://handle.uws.edu.au:8081/1959.7/548862
M3 - Conference Paper
SP - 357
EP - 364
BT - Proceedings of the 15th International Symposium on Space Terahertz Technology, April 27-29, 2004, Hotel Northampton, Northampton, Massachusetts
PB - National Radio Astronomy Observatory
T2 - International Symposium on Space Terahertz Technology
Y2 - 1 January 2008
ER -
Nikola T, Stacey GJ, Oberst TE, Parshley SC, Stark AA, Tothill N et al. SPIFI : The South Pole Imaging Fabry-Perot Interferometer on AST/RO. In Proceedings of the 15th International Symposium on Space Terahertz Technology, April 27-29, 2004, Hotel Northampton, Northampton, Massachusetts. National Radio Astronomy Observatory. 2004. p. 357-364
