Two bolometer Arrays for far-infrared and submillimeter astronomy

被引：1

作者：

Silverberg, RF ^{[1
]}

Allen, CA ^{[1
]}

Babu, SR ^{[1
]}

Benford, DJ ^{[1
]}

Chuss, DT ^{[1
]}

Dotson, JL ^{[1
]}

Dowell, CD ^{[1
]}

Harper, DA ^{[1
]}

Jhabvala, MD ^{[1
]}

Loewenstein, RF ^{[1
]}

Moseley, SH ^{[1
]}

Staguhn, JG ^{[1
]}

Voellmer, G ^{[1
]}

Wollack, EJ ^{[1
]}

机构：

[1] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

来源：

MILLIMETER AND SUBMILLIMETER DETECTORS FOR ASTRONOMY II | 2004年 / 5498卷

关键词：

bolometer; far-infrared; sub-millimeter; detector arrays; instrumentation; CSO; SOFIA;

D O I：

10.1117/12.552422

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We describe the development, construction, and testing of two 384 element arrays of ion-implanted semi-conducting cryogenic bolometers designed for use in far-infrared and submillimeter cameras. These two dimensional arrays are assembled from a number of 32 element linear arrays of monolithic Pop-Up bolometer Detectors (PUD) developed at NASA/Goddard Space Flight Center. PUD technology allows the construction of large, high filling factor, arrays that make efficient use of available focal plane area in far-infrared and submillimeter astronomical instruments. Such arrays can be used to provide a significant increase in mapping speed over smaller arrays. A prototype array has been delivered and integrated into a ground-based camera, the Submillimeter High Angular Resolution Camera (SHARC II), a facility instrument at the Caltech Submillimeter Observatory (CSO). A second array has recently been delivered for integration into the High-resolution Airborne Widebandwidth Camera (HAWC), a far-infrared imaging camera for the Stratospheric Observatory for Infrared Astronomy (SOFIA). HAWC is scheduled for commissioning in 2005.

引用

页码：187 / 195

页数：9

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