The Spitzer warm mission science prospects

被引：0

作者：

Stauffer, John R. ^{[1
]}

Mannings, Vincent ^{[1
]}

Levine, Deborah ^{[1
]}

Chary, Ranga Ram ^{[1
]}

Wilson, Gillian ^{[1
]}

Lacy, Mark ^{[1
]}

Grillmair, Carl ^{[1
]}

Carey, Sean ^{[1
]}

Stolovy, Susan ^{[1
]}

Ciardi, David ^{[2
]}

Hora, Joe ^{[3
]}

机构：

[1] CALTECH, Spitzer Sci Ctr, 314-6, Pasadena, CA 91125 USA

[2] CALTECH, Infrared Proc & Anal Ctr, Pasadena, CA 91125 USA

[3] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 01238 USA

来源：

SCIENCE OPPORTUNITIES FOR THE WARM SPITZER MISSION WORKSHOP | 2007年 / 943卷

基金：

美国国家科学基金会; 美国国家航空航天局;

关键词：

Spitzer Space Telescope; infrared astronomical observations; exoplanets; AGN; galaxy clusters; asteroids; star-formation regions; protostars;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

After exhaustion of its cryogen, the Spitzer Space telescope will still have a fully functioning two-channel mid-IR camera that will have sensitivities better than any other ground or spacebased telescopes until the launch of JWST. This document provides a description of the expected capabilities of Spitzer during its warm mission phase, and provides brief descriptions of several possible very large science programs that could be conducted. This information is intended to serve as input to a wide ranging discussion of the warm mission science, leading up to the Warm Mission Workshop in June 2007.

引用

页码：43 / +

页数：4

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