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Beam profile for the Herschel-SPIRE Fourier transform spectrometer. 2013
Gibion Makiwa, and
David A Naylor, and
Marc Ferlet, and
Carl Salji, and
Bruce Swinyard, and
Edward Polehampton, and
Matthijs H D van der Wiel
Institute for Space Imaging Science, Department of Physics and Astronomy, University of Lethbridge, Lethbridge, Alberta, Canada. gibion.makiwa@uleth.ca
One of the instruments on board the Herschel Space Observatory is the Spectral and Photometric Imaging Receiver (SPIRE). SPIRE employs a Fourier transform spectrometer with feed-horn-coupled bolometers to provide imaging spectroscopy. To interpret the resultant spectral images requires knowledge of the wavelength-dependent beam, which in the case of SPIRE is complicated by the use of multimoded feed horns. In this paper we describe a series of observations and the analysis conducted to determine the wavelength dependence of the SPIRE spectrometer beam profile.
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