The Herschel submm space observatory

被引：0

作者：

Clavel, J ^{[1
]}

机构：

[1] ESA, Astrophys Miss Div, Res & Sci Support Dpt, Estec, NL-2201 AZ Noordwijk, Netherlands

来源：

INTERPLAY AMONG BLACK HOLES, STARS AND ISM IN GALACTIC NUCLEI | 2004年 / 222期

关键词：

D O I：

10.1017/S1743921304003254

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The "Herschel Space Observatory" is an ESA mission to perform imaging photometry and spectroscopy in the far-IR & submm 57-670 mu m range. It carries a 3.5 m diameter radiatively cooled telescope. The scientific instruments - two cameras/medium resolution spectrometers (PACS and SPIRE) and a very high resolution heterodyne spectrometer (HIFI) - are housed in a superfluid helium cryostat. Herschel will be placed in orbit around the Earth-Sun L2 point in 2007 and will operate for a minimum of 3 years. Roughly 2/3 of the observing time is open to the general astronomical community through a competitive proposal procedure.

引用

页码：553 / 554

页数：2

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