Abstract
The Stratospheric TeraHertz Observatory (STO) is a NASA funded, Long Duration Balloon (LDB) experiment designed to address a key problem in modern astrophysics: understanding the Life Cycle of the Interstellar Medium (ISM). STO will survey a section of the Galactic plane in the dominant interstellar cooling line [C II] (1.9 THz) and the important star formation tracer [N II] (1.46 THz) at ~1 arc minute angular resolution, sufficient to spatially resolve atomic, ionic and molecular clouds at 10 kpc. The science flight instrument package hosts four [CII] and four [NII] HEB receivers. There is also one 492 GHz Schottky receiver for observing the [CI] line. In this paper we discuss preparations for the scheduled Antarctic science flight in December 2011.
Original language | English (US) |
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Pages | 159-161 |
Number of pages | 3 |
State | Published - 2011 |
Event | 22nd International Symposium on Space Terahertz Technology 2011, ISSTT 2011 - Tucson, AZ, United States Duration: Apr 25 2011 → Apr 28 2011 |
Other
Other | 22nd International Symposium on Space Terahertz Technology 2011, ISSTT 2011 |
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Country/Territory | United States |
City | Tucson, AZ |
Period | 4/25/11 → 4/28/11 |
ASJC Scopus subject areas
- Computer Networks and Communications
- Space and Planetary Science
- Electrical and Electronic Engineering
- Atomic and Molecular Physics, and Optics
- Radiation