Instruments with Many Dichroic Mirrors and CCDs

被引：0

作者：

Doi, N. ^{[1
]}

Hayano, J. ^{[1
]}

Utsunomiya, H. ^{[1
]}

Ihara, Y. ^{[1
]}

Tokita, K. ^{[1
]}

Takanashi, N. ^{[1
]}

Sako, S. ^{[1
]}

Okamura, S. ^{[2
]}

Morokuma, T. ^{[3
]}

Furusawa, H. ^{[3
]}

Komiyama, Y. ^{[3
]}

Yagi, M. ^{[3
]}

Okada, N. ^{[3
]}

Arai, A.

Uemura, M.

Kawabata, K.

Yamashita, T.

Osugi, T.

Abe, M.

Hasegawa, S.

机构：

[1] Univ Tokyo, Grad Sch Sci, Inst Astron, 2-21-1 Osawa, Tokyo 1810015, Japan

[2] Univ Tokyo, Grad Sch Sci, Dept Astron, Tokyo 1130033, Japan

[3] Natl Inst Nat Sci, Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan

来源：

PANORAMIC VIEWS OF GALAXY FORMATION AND EVOLUTION, PROCEEDINGS | 2008年 / 399卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We developed a 15-band simultaneous imager called a Dichroic Mirror Camera (DMC) using many dichroic mirrors. DNIC covers a wide optical wavelength range (390-930 nm) in 15 intermediate bands. We successfully got the. first light at the 1.5-m Kanata, telescope in May 2007, The field of view is about. 11 aremin in diameter with 0.27 aresec/pixel. Optical performance of DMC was satisfactory to carry out astronomical observations. We also discuss possible extensions of DNIC as a spectrograph with a grisin mode and multi-bands Fabry-Perot mode as well as future photometric redshift surveys.

引用

页码：491 / +

页数：2

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