UKIDSS: Surveying the Sky in the Near-IR

被引：0

作者：

Gonzalez-Solares, E. A. ^{[1
]}

Venemans, B. P. ^{[1
]}

McMahon, R. G. ^{[1
]}

Warren, S. J. ^{[2
]}

Mortlock, D. J. ^{[2
]}

Patel, M. ^{[2
]}

Hewett, P. C. ^{[1
]}

Dye, S. ^{[3
]}

Sharp, R. G. ^{[4
]}

机构：

[1] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England

[2] Imperial Coll London, Astrophys Grp, Blackett Lab, London SW7 2AZ, England

[3] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, Wales

[4] Anglo Australian Observ, Epping, NSW 1710, Australia

来源：

HIGHLIGHTS OF SPANISH ASTROPHYSICS V | 2010年

关键词：

PROBE WMAP OBSERVATIONS; Z-SIMILAR-TO-6; QUASARS; REIONIZATION; DISCOVERY; EVOLUTION; DENSITY; EPOCH;

D O I：

10.1007/978-3-642-11250-8_10

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The UKIRT Infrared Deep Sky Survey (UKIDSS) is observing about 7,000 square degrees of the northern sky in the near-IR. Summed together it is 12 times larger in effective volume than the 2MASS survey. The scientific aims of UKIDSS include the detection of the nearest and faintest substellar objects and brown dwarfs, probe the substellar initial mass function, detect clusters of galaxies at z similar to 2 and detect high redshift quasars at z similar to 6-7. We give here a short introduction to UKIDSS focusing mainly on the search for high-z quasars.

引用

页码：111 / +

页数：3

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