Proceedings Paper
Balloon-Borne Observations Of The Cygnus Region In The Far Infrared| Format | Member Price | Non-Member Price |
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Paper Abstract
A balloon-borne far-infrared telescope has been designed and built to observe the infrared emission from the Cygnus region in the galactic plane between 120 μm and 300 μm wavelength. The system performance, objects as well as results of the first flight in September 1988 will be discussed.
Paper Details
Date Published: 18 November 1989
PDF: 2 pages
Proc. SPIE 1039, 13th Intl Conf on Infrared and Millimeter Waves, (18 November 1989); doi: 10.1117/12.978338
Published in SPIE Proceedings Vol. 1039:
13th Intl Conf on Infrared and Millimeter Waves
Richard J. Temkin, Editor(s)
PDF: 2 pages
Proc. SPIE 1039, 13th Intl Conf on Infrared and Millimeter Waves, (18 November 1989); doi: 10.1117/12.978338
Show Author Affiliations
C. G. Degiacomi, Infrared Physics Laboratory (Switzerland)
A. Holenstein, Infrared Physics Laboratory (Switzerland)
A. Holenstein, Infrared Physics Laboratory (Switzerland)
F. K. Kneubuhl, Infrared Physics Laboratory (Switzerland)
D. Huguenin, Geneva Observatory (Switzerland)
D. Huguenin, Geneva Observatory (Switzerland)
Published in SPIE Proceedings Vol. 1039:
13th Intl Conf on Infrared and Millimeter Waves
Richard J. Temkin, Editor(s)
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