HIFI stability as measured during ILT phase
Paper i proceeding, 2008
We present here the stability results of the high frequency heterodyne instrument (HIFI), to be flown on the Herschel space observatory. The measurements were taken as part of the instrument level tests (ILT) in the spring of 2007. Herschel is ESA's fourth cornerstone mission in the Horizon 2000+ program, and aims at observations in the Far-InfraRed and sub-millimeter wavelength region. HIFI itself is one of three instruments onboard Herschel. The other two being PACS, the photodetector array camera and spectrometer, and SPIRE, the spectral and photometric imaging receiver.
Författare
J. Kooi
California Institute of Technology (Caltech)
V. Ossenkopf
Universität zu Köln
Netherlands Institute for Space Research (SRON)
Michael Olberg
Chalmers, Institutionen för radio- och rymdvetenskap
R. Shipman
Rijksuniversiteit Groningen
R. Schieder
Universität zu Köln
D. Teyssier
European Space Astronomy Centre (ESAC)
19th International Symposium on Space Terahertz Technology, ISSTT 2008; Groningen; Netherlands; 28 April 2008 through 30 April 2008
92-102
Ämneskategorier
Astronomi, astrofysik och kosmologi