DocumentCode
2644513
Title
Application of Millimeter Wave Receivers to Astronomy
Author
Phillips, T.G. ; Jefferts, K.B.
Volume
74
Issue
1
fYear
1974
fDate
12-14 June 1974
Firstpage
116
Lastpage
116
Abstract
Millimeter wave receivers are discussed from the point of view of applications of line astronomy. A heterodyne bolometer system is described which has a noise temperature of 300/spl deg/K at 230 GHz. It is expected that these receivers will extend the range of radio line astronomy to about 500 GHz.
Keywords
Astronomy; Bolometers; Educational institutions; Receivers; Temperature;
fLanguage
English
Publisher
ieee
Conference_Titel
Microwave Symposium Digest, 1974 S-MTT International
Conference_Location
Atlanta, Georgia, USA
Type
conf
DOI
10.1109/MWSYM.1974.1123613
Filename
1123613
Link To Document