Pan-STARRS - A large synoptic survey telescope array

被引：677

作者：

Kaiser, N ^{[1
]}

Aussel, H ^{[1
]}

Burke, B ^{[1
]}

Boesgaard, H ^{[1
]}

Chambers, K ^{[1
]}

Chun, M ^{[1
]}

Heasley, J ^{[1
]}

Hodapp, K ^{[1
]}

Hunt, B ^{[1
]}

Jedicke, R ^{[1
]}

Jewitt, D ^{[1
]}

Kudritzki, R ^{[1
]}

Luppino, G ^{[1
]}

Maberry, M ^{[1
]}

Magnier, E ^{[1
]}

Monet, D ^{[1
]}

Onaka, P ^{[1
]}

Pickles, A ^{[1
]}

Rhoads, PH ^{[1
]}

Simon, T ^{[1
]}

Szalay, A ^{[1
]}

Szapudi, I ^{[1
]}

Tholen, D ^{[1
]}

Tonry, J ^{[1
]}

Waterson, M ^{[1
]}

Wick, A ^{[1
]}

机构：

[1] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA

来源：

SURVEY AND OTHER TELESCOPE TECHNOLOGIES AND DISCOVERIES | 2002年 / 4836卷

关键词：

wide-field imaging; survey telescopes; large-format CCDs; near earth asteroids;

D O I：

10.1117/12.457365

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The IfA and collaborators are embarking on a project to develop a 4-telescope synoptic survey instrument. While somewhat smaller than the 6.5m class telescope envisaged by the decadal review in their proposal for a LSST, this facility will nonetheless be able to accomplish many of the LSST science goals. In this paper we will describe the motivation for a 'distributed aperture' approach for the LSST, the current concept for Pan-STARRS - a pilot project for the LSST proper - and its performance goals and science reach. We will also discuss how the facility may be expanded.

引用

页码：154 / 164

页数：11

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