Beam profile for the Herschel-SPIRE Fourier transform spectrometer

被引：34

作者：

Makiwa, Gibion ^{[1
]}

Naylor, David A. ^{[1
]}

Ferlet, Marc ^{[2
]}

Salji, Carl ^{[3
]}

Swinyard, Bruce ^{[2
,3
]}

Polehampton, Edward ^{[1
,2
]}

van der Wiel, Matthijs H. D. ^{[1
]}

机构：

[1] Univ Lethbridge, Dept Phys & Astron, Inst Space Imaging Sci, Lethbridge, AB T1K 3M4, Canada

[2] Rutherford Appleton Lab, RAL Space, Didcot OX11 0QX, Oxon, England

[3] UCL, Dept Phys & Astron, London WC1E 6BT, England

来源：

APPLIED OPTICS | 2013年 / 52卷 / 16期

关键词：

COUPLED BOLOMETER ARRAYS; INSTRUMENT; MISSION; DESIGN; SPECTROSCOPY; PERFORMANCE;

D O I：

10.1364/AO.52.003864

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

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. (C) 2013 Optical Society of America

引用

页码：3864 / 3875

页数：12

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