The LSST sensor technologies studies

被引：0

作者：

Geary, J. ^{[1
]}

Figer, D. ^{[2
]}

Gilmore, D. K. ^{[3
]}

O'Connor, P. ^{[4
]}

Oliver, J. ^{[5
]}

Radeka, V. ^{[4
]}

Stubbs, C. ^{[6
]}

Takas, P. ^{[4
]}

Tyson, J. A. ^{[7
]}

机构：

[1] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA

[2] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA

[3] Stanford Linear Accelerator Ctr, Stanford, CA 94309 USA

[4] Brookhaven Natl Lab, Upton, NY 11973 USA

[5] Harvard Univ, Lab Particle Phy Cosmol, Cambridge, MA 02138 USA

[6] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA

[7] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA

来源：

HIGH ENERGY, OPTICAL, AND INFRARED DETECTORS FOR ASTRONOMY II | 2006年 / 6276卷

基金：

美国国家科学基金会;

关键词：

LSST; sensor; imager; CCD; CMOS;

D O I：

10.1117/12.673291

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The LSST project has embarked on an aggressive new program to develop the next generation of silicon imagers for the visible and near-IR spectral regions. In order to better understand and solve some of the technology issues prior to development and mass-production for the huge LSST focal plane, a number of contracts have been written to imager firms to explore specific areas of technology uncertainty. We expect that these study contracts will do much toward reducing risk and uncertainty going into the next phase of development, the prototype production of the final large LSST imager.

引用

页数：8