K-band galaxy counts in the south galactic pole region

被引:43
作者
Minezaki, T
Kobayashi, Y
Yoshii, Y
Peterson, BA
机构
[1] Natl Astron Observ, Tokyo 181, Japan
[2] Univ Tokyo, Fac Sci, Inst Astron, Tokyo 181, Japan
[3] Australian Natl Univ, Mt Stromlo & Siding Spring Observ, Inst Adv Studies, Weston, ACT 2611, Australia
关键词
cosmology; observations; galaxies; evolution; photometry; statistics; Galaxy; structure; infrared; surveys;
D O I
10.1086/305194
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present new K-band galaxy number counts from K = 13 to 20.5 obtained from K'-band surveys in the south galactic pole region, which cover 180.8 arcmin(2) to a limiting magnitude of K = 19 and 2.21 arcmin(2) to K = 21. These are currently the most precise K-band galaxy counts at 17.5 < K < 19.0 because the area of coverage is largest among the existing surveys for this magnitude range. The completeness and photometry corrections are estimated from the recovery of simulated galaxy and stellar profiles added to the obtained field image. Many simulations were carried out to construct a probability matrix that corrects the galaxy counts at the faint-end magnitudes of the surveys so the corrected counts can be compared with other observations. The K-band star counts in the south galactic pole region to K = 17.25 are also presented for use to constrain the vertical structure of the Galaxy.
引用
收藏
页码:111 / +
页数:9
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