The orthogonal-transfer array: A new CCD architecture for astronomy

被引：23

作者：

Burke, B ^{[1
]}

Tonry, J ^{[1
]}

Cooper, M ^{[1
]}

Luppino, G ^{[1
]}

Jacoby, G ^{[1
]}

Bredthauer, R ^{[1
]}

Boggs, K ^{[1
]}

Lesser, M ^{[1
]}

Onaka, P ^{[1
]}

Young, D ^{[1
]}

Doherty, P ^{[1
]}

Craig, D ^{[1
]}

机构：

[1] MIT, Lincoln Lab, Lexington, MA 02420 USA

来源：

OPTICAL AND INFRARED DETECTORS FOR ASTRONOMY | 2004年 / 5499卷

关键词：

CCD; OTCCD; orthogonal-transfer CCD; Pan-STARRS; WIYN; tip tilt;

D O I：

10.1117/12.562490

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

The orthogonal-transfer array (OTA) is a new CCD architecture designed to provide wide-field tip-tilt correction of astronomical images. The device consists of an 8x8 array of small (similar to500x500 pixels) orthogonal-transfer CCDs (OTCCD) with independent addressing and readout of each OTCCD. This approach enables an optimum tip-tilt correction to be applied independently to each OTCCD across the focal plane. The first design of this device has been carried out at MIT Lincoln Laboratory in support of the Pan-STARRS program with a collaborative parallel effort at Semiconductor Technology Associates (STA) for the WIYN Observatory. The two versions of this device are functionally compatible and share a common pinout and package. The first wafer lots are complete at Lincoln and at Dalsa and are undergoing wafer probing.

引用

页码：185 / 192

页数：8

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