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首页> 外文会议>Conference on Survey and Other Telescope Technologies and Discoveries; Aug 27-28, 2002; Waikoloa, Hawaii, USA >Scientific goals of the UKIRT Infrared Deep Sky Survey
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Scientific goals of the UKIRT Infrared Deep Sky Survey

机译：UKIRT红外深空调查的科学目标

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摘要

UKIDSS is the next generation near-infrared sky survey. The survey will commence in early 2004, and over 7 years will collect 100 times as many photons as 2MASS. UKIDSS will use the UKIRT Wide Field Camera to survey 7500 square degrees of the northern sky, extending over both high and low Galactic latitudes, in JHK to K=18.5 (over three magnitudes deeper than 2MASS). UKIDSS will be the true near-infrared counterpart to the Sloan survey, and will produce as well a panoramic clear atlas of the Galactic plane. In fact UKIDSS is made up of five surveys and includes two deep extra-Galactic elements, one covering 35 square degrees to K=21, and the other reaching K=23 over 0.77 square degrees. This paper provides the details of the five UKIDSS surveys and describes the main science goals.
机译：UKIDSS是下一代近红外天空调查。这项调查将于2004年初开始，超过7年的时间将收集到2MASS数量100倍的光子。 UKIDSS将使用UKIRT广角摄像机在JHK的高空和低银河纬度上勘测7500平方公里的北部天空，达到K = 18.5（比2MASS深度高三个量级）。 UKIDSS将是斯隆（Sloan）调查的真正近红外对口，并且还将制作银河系平面全景图集。实际上，UKIDSS由五项调查组成，包括两个深层银河系元素，一个覆盖35平方度，到K = 21，另一个覆盖K = 23，覆盖0.77平方米。本文提供了五项UKIDSS调查的详细信息，并描述了主要的科学目标。

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