The Herschel ATLAS

The Herschel ATLAS
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DOI:
10.1086/653086
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发表时间:
2009-10
影响因子:
3.5
通讯作者:
S. Eales;L. Dunne;D. Clements;A. Cooray;G. Zotti;S. Dye;R. Ivison;M. Jarvis;G. Lagache
S. Eales;L. Dunne;D. Clements;A. Cooray;G. Zotti;S. Dye;R. Ivison;M. Jarvis;G. Lagache
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
S. Eales;L. Dunne;D. Clements;A. Cooray;G. Zotti;S. Dye;R. Ivison;M. Jarvis;G. Lagache

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赫歇尔ATLAS是赫歇尔空间天文台将进行的最大的开放时间关键项目。它将在五个远红外和亚毫米波段调查570度2的河外天空,比所有其他赫歇尔河外调查的总和大4倍。我们描述的调查,互补的多波长数据集,将结合赫歇尔数据,和六个主要的科学计划,我们正在进行。使用新的模型的基础上以前的亚毫米调查的星系,我们提出了预测的属性的ATLAS源在其他波段。
The Herschel ATLAS is the largest open-time key project that will be carried out on the Herschel Space Observatory. It will survey 570 deg2 of the extragalactic sky, 4 times larger than all the other Herschel extragalactic surveys combined, in five far-infrared and submillimeter bands. We describe the survey, the complementary multiwavelength data sets that will be combined with the Herschel data, and the six major science programs we are undertaking. Using new models based on a previous submillimeter survey of galaxies, we present predictions of the properties of the ATLAS sources in other wave bands.