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Far-Infrared Astronomy with the CO N+ Deuterium Observations Receiver (CONDOR)

Published online by Cambridge University Press:  04 October 2008

C. Kramer ,
S. Aalto ,
R. Simon ,
M.C. Wiedner ,
F. Bielau ,
M. Emprechtinger ,
O. Ricken ,
N. Volgenau ,
G. Wieching  and
U.U. Graf
...Show all authors
M.C. Wiedner
Affiliation:
1. Physikalische Institut, Universität zu Köln, Germany
F. Bielau
Affiliation:
1. Physikalische Institut, Universität zu Köln, Germany
M. Emprechtinger
Affiliation:
1. Physikalische Institut, Universität zu Köln, Germany
O. Ricken
Affiliation:
1. Physikalische Institut, Universität zu Köln, Germany
N. Volgenau
Affiliation:
1. Physikalische Institut, Universität zu Köln, Germany
G. Wieching
Affiliation:
1. Physikalische Institut, Universität zu Köln, Germany
U.U. Graf
Affiliation:
1. Physikalische Institut, Universität zu Köln, Germany
C.E. Honingh
Affiliation:
1. Physikalische Institut, Universität zu Köln, Germany
K. Jacobs
Affiliation:
1. Physikalische Institut, Universität zu Köln, Germany
J. Stutzki
Affiliation:
1. Physikalische Institut, Universität zu Köln, Germany
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Abstract

The CO N+ Deuterium Observations Receiver (CONDOR) is one of the very fewheterodyne receivers operational between 1.25 and 1.53 THz. It has successfullyobtained first-light observations on APEX and is currently being modified tofly as the low frequency channel of GREAT on SOFIA.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 31: Far-Infrared Workshop 2007 , 2008 , pp. 215 - 216
Copyright
© EAS, EDP Sciences, 2008

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References

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Munoz, P., et al., 2004, “Fifteenth International Symposium on Space Terahertz Technology”, Amherst
Volgenau, N.H., et al., 2008, A&A, submitted
Wiedner, M.C., et al., 2006, A&A, 454, L33