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CONDOR – A heterodyne receiver at 1.25-1.5 THz

Published online by Cambridge University Press:  01 August 2006

M. C. Wiedner ,
G. Wieching ,
F. Bielau ,
M. Emprechtinger ,
U. U. Graf ,
C. E. Honingh ,
K. Jacobs ,
D. Paulussen ,
K. Rettenbacher  and
N. H. Volgenau
M. C. Wiedner
Affiliation:
I. Physikalisches Institut, Universität zu Köln, 50937 Köln, Germany
G. Wieching
Affiliation:
I. Physikalisches Institut, Universität zu Köln, 50937 Köln, Germany
F. Bielau
Affiliation:
I. Physikalisches Institut, Universität zu Köln, 50937 Köln, Germany
M. Emprechtinger
Affiliation:
I. Physikalisches Institut, Universität zu Köln, 50937 Köln, Germany
U. U. Graf
Affiliation:
I. Physikalisches Institut, Universität zu Köln, 50937 Köln, Germany
C. E. Honingh
Affiliation:
I. Physikalisches Institut, Universität zu Köln, 50937 Köln, Germany
K. Jacobs
Affiliation:
I. Physikalisches Institut, Universität zu Köln, 50937 Köln, Germany
D. Paulussen
Affiliation:
I. Physikalisches Institut, Universität zu Köln, 50937 Köln, Germany
K. Rettenbacher
Affiliation:
I. Physikalisches Institut, Universität zu Köln, 50937 Köln, Germany
N. H. Volgenau
Affiliation:
I. Physikalisches Institut, Universität zu Köln, 50937 Köln, Germany
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The CON+Deuterium Observations Receiver (CONDOR) is a heterodyne receiver that operates between 1250–1530 GHz. Its primary goal is to observe star-forming regions in CO, N+, and H2D+ emission.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S237: Triggered Star Formation in a Turbulent ISM , August 2006 , pp. 495
Copyright
Copyright © International Astronomical Union 2007

References

Muñoz, P.P., Bedorf, S., Brandt, M. et al. 2004, SPIE 5498, 834Google Scholar
Wiedner, M.C., Wieching, G., Bielau, F. et al. 2006, A&A 454, L33Google Scholar