First astronomical images obtained with an array of multiplexed superconducting bolometers

被引：2
|
作者：
Staguhn, JG [1 ]
Benford, DJ
Moseley, SH
Allen, CA
Kennedy, CR
Lefranc, S
Maher, SF
Pajot, F
Rioux, C
Shafer, RA
Voellmer, GM
机构：
[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
[2] SSAI, Lanham, MD 20706 USA
[3] Univ Notre Dame, Notre Dame, IN 46556 USA
[4] Inst Astrophys Spatiale, Orsay, France
来源：
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2006年 / 559卷 / 02期
关键词：
bolometers; detectors; multiplexers; sub-mm instruments; spectrometers;
D O I：
10.1016/j.nima.2005.12.087
中图分类号：
TH7 [仪器、仪表];
学科分类号：
0804 ; 080401 ; 081102 ;
摘要：
We present multicolor images of Jupiter observed in the 350 mu m band with the first deployed astronomical instrument to use multiplexed superconducting bolometers. The Fabry-Perot Interferometer Bolometer Research Experiment (FIBRE) is a broadband submillimeter spectrometer that made these images in July 2004 at the Caltech Submillimeter Observatory (CSO). FIBREs detectors are superconducting bilayer transition edge sensor (TES) bolometers read out by a SQUID multiplexer. An order-sorted Fabry-Perot provides illumination of a 16-element linear bolometer array, resulting in five orders at a spectral resolution R of 1200 covering a band of of the observed wavelength. The optics permit these orders to be scanned to cover the entirety of either the 350 or 450 mu m bands. (c) 2006 Elsevier B.V. All rights reserved.
引用
收藏
页码：602 / 604
页数：3
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