SEEDS: Target Selection for Open Clusters and Moving Groups

被引：0

作者：

Yamamoto, K. ^{[1
]}

Matsuo, T.

McElwain, M. ^{[2
]}

Tamura, M. ^{[3
]}

Morishita, H. ^{[1
]}

Nakashima, A. ^{[1
]}

Shibai, H. ^{[4
]}

Fukagawa, M. ^{[4
]}

Kato, E. ^{[4
]}

Kanoh, T. ^{[4
]}

Itoh, Yusuke ^{[4
]}

Kaneko, Y. ^{[4
]}

Shimoura, M. ^{[4
]}

Itoh, Yoichi ^{[5
]}

Funayama, H. ^{[4
]}

Hashiguchi, T. ^{[4
]}

机构：

[1] Nagoya Univ, Sch Sci, Dept Phys, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648602, Japan

[2] Princeton Univ, Astrophys Sci, Princeton, NJ 08544 USA

[3] Natl Inst Nat Sci, Natl Astron Observ Japan, Div Opt &Infrared Astronom, Mitaka, Tokyo 1818588, Japan

[4] Osaka Univ, Grad Sch Sci, Dept Earth & Space Sci, Osaka 5600043, Japan

[5] Kobe Univ, Grad Sch Sci & Technol, Kobe, Hyogo, Japan

来源：

EXOPLANETS AND DISKS: THEIR FORMATION AND DIVERSITY | 2009年 / 1158卷

关键词：

exoplanet; Subaru telescope; HiCIAO; SEEDS;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We selected the target stars for the Subaru Strategic Exploration of Exoplanets and Disks (SEEDS) with the High-contrast Coronagraphic Imager for Adaptive Optics (HiCIAO/AO188) observations from the members of open clusters and moving groups. For this selection, we defined the criteria for open clusters and moving groups. Using those selection criteria, we made a target list for open clusters and moving groups. The number of target stars selected is 50 from each category. As a result, the target stars for the open cluster category were selected only from the Pleiades, and those for the moving groups were from six different moving groups. We calculated the expected number of exoplanet detections by HiCIAO and AO188 (to be used on Subaru) by assuming the exoplanet formation probability. The expected number of the direct exoplanet detection is 28 in this category.

引用

页码：273 / +

页数：2

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